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  • American Association for the Advancement of Science (AAAS)  (531)
  • Springer Science + Business Media
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  • 1
    Publikationsdatum: 2012-01-17
    Beschreibung: Gamma-ray binaries are stellar systems containing a neutron star or black hole, with gamma-ray emission produced by an interaction between the components. These systems are rare, even though binary evolution models predict dozens in our Galaxy. A search for gamma-ray binaries with the Fermi Large Area Telescope (LAT) shows that 1FGL J1018.6-5856 exhibits intensity and spectral modulation with a 16.6-day period. We identified a variable x-ray counterpart, which shows a sharp maximum coinciding with maximum gamma-ray emission, as well as an O6V((f)) star optical counterpart and a radio counterpart that is also apparently modulated on the orbital period. 1FGL J1018.6-5856 is thus a gamma-ray binary, and its detection suggests the presence of other fainter binaries in the Galaxy.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Fermi LAT Collaboration -- Ackermann, M -- Ajello, M -- Ballet, J -- Barbiellini, G -- Bastieri, D -- Belfiore, A -- Bellazzini, R -- Berenji, B -- Blandford, R D -- Bloom, E D -- Bonamente, E -- Borgland, A W -- Bregeon, J -- Brigida, M -- Bruel, P -- Buehler, R -- Buson, S -- Caliandro, G A -- Cameron, R A -- Caraveo, P A -- Cavazzuti, E -- Cecchi, C -- Celik, O -- Charles, E -- Chaty, S -- Chekhtman, A -- Cheung, C C -- Chiang, J -- Ciprini, S -- Claus, R -- Cohen-Tanugi, J -- Corbel, S -- Corbet, R H D -- Cutini, S -- de Luca, A -- den Hartog, P R -- de Palma, F -- Dermer, C D -- Digel, S W -- do Couto e Silva, E -- Donato, D -- Drell, P S -- Drlica-Wagner, A -- Dubois, R -- Dubus, G -- Favuzzi, C -- Fegan, S J -- Ferrara, E C -- Focke, W B -- Fortin, P -- Fukazawa, Y -- Funk, S -- Fusco, P -- Gargano, F -- Gasparrini, D -- Gehrels, N -- Germani, S -- Giglietto, N -- Giordano, F -- Giroletti, M -- Glanzman, T -- Godfrey, G -- Grenier, I A -- Grove, J E -- Guiriec, S -- Hadasch, D -- Hanabata, Y -- Harding, A K -- Hayashida, M -- Hays, E -- Hill, A B -- Hughes, R E -- Johannesson, G -- Johnson, A S -- Johnson, T J -- Kamae, T -- Katagiri, H -- Kataoka, J -- Kerr, M -- Knodlseder, J -- Kuss, M -- Lande, J -- Longo, F -- Loparco, F -- Lovellette, M N -- Lubrano, P -- Mazziotta, M N -- McEnery, J E -- Michelson, P F -- Mitthumsiri, W -- Mizuno, T -- Monte, C -- Monzani, M E -- Morselli, A -- Moskalenko, I V -- Murgia, S -- Nakamori, T -- Naumann-Godo, M -- Norris, J P -- Nuss, E -- Ohno, M -- Ohsugi, T -- Okumura, A -- Omodei, N -- Orlando, E -- Ozaki, M -- Paneque, D -- Parent, D -- Pesce-Rollins, M -- Pierbattista, M -- Piron, F -- Pivato, G -- Porter, T A -- Raino, S -- Rando, R -- Razzano, M -- Reimer, A -- Reimer, O -- Ritz, S -- Romani, R W -- Roth, M -- Saz Parkinson, P M -- Sgro, C -- Siskind, E J -- Spandre, G -- Spinelli, P -- Suson, D J -- Takahashi, H -- Tanaka, T -- Thayer, J G -- Thayer, J B -- Thompson, D J -- Tibaldo, L -- Tinivella, M -- Torres, D F -- Tosti, G -- Troja, E -- Uchiyama, Y -- Usher, T L -- Vandenbroucke, J -- Vianello, G -- Vitale, V -- Waite, A P -- Winer, B L -- Wood, K S -- Wood, M -- Yang, Z -- Zimmer, S -- Coe, M J -- Di Mille, F -- Edwards, P G -- Filipovic, M D -- Payne, J L -- Stevens, J -- Torres, M A P -- New York, N.Y. -- Science. 2012 Jan 13;335(6065):189-93. doi: 10.1126/science.1213974.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22246769" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
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  • 2
    Publikationsdatum: 2012-11-03
    Beschreibung: The light emitted by stars and accreting compact objects through the history of the universe is encoded in the intensity of the extragalactic background light (EBL). Knowledge of the EBL is important to understand the nature of star formation and galaxy evolution, but direct measurements of the EBL are limited by galactic and other foreground emissions. Here, we report an absorption feature seen in the combined spectra of a sample of gamma-ray blazars out to a redshift of z approximately 1.6. This feature is caused by attenuation of gamma rays by the EBL at optical to ultraviolet frequencies and allowed us to measure the EBL flux density in this frequency band.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Ackermann, M -- Ajello, M -- Allafort, A -- Schady, P -- Baldini, L -- Ballet, J -- Barbiellini, G -- Bastieri, D -- Bellazzini, R -- Blandford, R D -- Bloom, E D -- Borgland, A W -- Bottacini, E -- Bouvier, A -- Bregeon, J -- Brigida, M -- Bruel, P -- Buehler, R -- Buson, S -- Caliandro, G A -- Cameron, R A -- Caraveo, P A -- Cavazzuti, E -- Cecchi, C -- Charles, E -- Chaves, R C G -- Chekhtman, A -- Cheung, C C -- Chiang, J -- Chiaro, G -- Ciprini, S -- Claus, R -- Cohen-Tanugi, J -- Conrad, J -- Cutini, S -- D'Ammando, F -- de Palma, F -- Dermer, C D -- Digel, S W -- do Couto e Silva, E -- Dominguez, A -- Drell, P S -- Drlica-Wagner, A -- Favuzzi, C -- Fegan, S J -- Focke, W B -- Franckowiak, A -- Fukazawa, Y -- Funk, S -- Fusco, P -- Gargano, F -- Gasparrini, D -- Gehrels, N -- Germani, S -- Giglietto, N -- Giordano, F -- Giroletti, M -- Glanzman, T -- Godfrey, G -- Grenier, I A -- Grove, J E -- Guiriec, S -- Gustafsson, M -- Hadasch, D -- Hayashida, M -- Hays, E -- Jackson, M S -- Jogler, T -- Kataoka, J -- Knodlseder, J -- Kuss, M -- Lande, J -- Larsson, S -- Latronico, L -- Longo, F -- Loparco, F -- Lovellette, M N -- Lubrano, P -- Mazziotta, M N -- McEnery, J E -- Mehault, J -- Michelson, P F -- Mizuno, T -- Monte, C -- Monzani, M E -- Morselli, A -- Moskalenko, I V -- Murgia, S -- Tramacere, A -- Nuss, E -- Greiner, J -- Ohno, M -- Ohsugi, T -- Omodei, N -- Orienti, M -- Orlando, E -- Ormes, J F -- Paneque, D -- Perkins, J S -- Pesce-Rollins, M -- Piron, F -- Pivato, G -- Porter, T A -- Raino, S -- Rando, R -- Razzano, M -- Razzaque, S -- Reimer, A -- Reimer, O -- Reyes, L C -- Ritz, S -- Rau, A -- Romoli, C -- Roth, M -- Sanchez-Conde, M -- Sanchez, D A -- Scargle, J D -- Sgro, C -- Siskind, E J -- Spandre, G -- Spinelli, P -- Stawarz, Lukasz -- Suson, D J -- Takahashi, H -- Tanaka, T -- Thayer, J G -- Thompson, D J -- Tibaldo, L -- Tinivella, M -- Torres, D F -- Tosti, G -- Troja, E -- Usher, T L -- Vandenbroucke, J -- Vasileiou, V -- Vianello, G -- Vitale, V -- Waite, A P -- Winer, B L -- Wood, K S -- Wood, M -- New York, N.Y. -- Science. 2012 Nov 30;338(6111):1190-2. doi: 10.1126/science.1227160. Epub 2012 Nov 1.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Deutsches Elektronen Synchrotron DESY, D-15738 Zeuthen, Germany.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23118013" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
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  • 3
    Publikationsdatum: 2012-06-23
    Beschreibung: In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The detection of close-in giant planets around other stars was the first clue that this pattern is not universal and that planets' orbits can change substantially after their formation. Here, we report another violation of the orbit-composition pattern: two planets orbiting the same star with orbital distances differing by only 10% and densities differing by a factor of 8. One planet is likely a rocky "super-Earth," whereas the other is more akin to Neptune. These planets are 20 times more closely spaced and have a larger density contrast than any adjacent pair of planets in the solar system.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Carter, Joshua A -- Agol, Eric -- Chaplin, William J -- Basu, Sarbani -- Bedding, Timothy R -- Buchhave, Lars A -- Christensen-Dalsgaard, Jorgen -- Deck, Katherine M -- Elsworth, Yvonne -- Fabrycky, Daniel C -- Ford, Eric B -- Fortney, Jonathan J -- Hale, Steven J -- Handberg, Rasmus -- Hekker, Saskia -- Holman, Matthew J -- Huber, Daniel -- Karoff, Christopher -- Kawaler, Steven D -- Kjeldsen, Hans -- Lissauer, Jack J -- Lopez, Eric D -- Lund, Mikkel N -- Lundkvist, Mia -- Metcalfe, Travis S -- Miglio, Andrea -- Rogers, Leslie A -- Stello, Dennis -- Borucki, William J -- Bryson, Steve -- Christiansen, Jessie L -- Cochran, William D -- Geary, John C -- Gilliland, Ronald L -- Haas, Michael R -- Hall, Jennifer -- Howard, Andrew W -- Jenkins, Jon M -- Klaus, Todd -- Koch, David G -- Latham, David W -- MacQueen, Phillip J -- Sasselov, Dimitar -- Steffen, Jason H -- Twicken, Joseph D -- Winn, Joshua N -- New York, N.Y. -- Science. 2012 Aug 3;337(6094):556-9. doi: 10.1126/science.1223269. Epub 2012 Jun 21.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA. jacarter@cfa.harvard.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22722249" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
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  • 4
    Publikationsdatum: 2012-11-01
    Beschreibung: Millisecond pulsars, old neutron stars spun up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled" rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive blind search of gamma-ray data from the Fermi Large Area Telescope (with partial constraints from optical data), we detected a 2.5-millisecond pulsar, PSR J1311-3430. This unambiguously explains a formerly unidentified gamma-ray source that had been a decade-long enigma, confirming previous conjectures. The pulsar is in a circular orbit with an orbital period of only 93 minutes, the shortest of any spin-powered pulsar binary ever found.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Pletsch, H J -- Guillemot, L -- Fehrmann, H -- Allen, B -- Kramer, M -- Aulbert, C -- Ackermann, M -- Ajello, M -- de Angelis, A -- Atwood, W B -- Baldini, L -- Ballet, J -- Barbiellini, G -- Bastieri, D -- Bechtol, K -- Bellazzini, R -- Borgland, A W -- Bottacini, E -- Brandt, T J -- Bregeon, J -- Brigida, M -- Bruel, P -- Buehler, R -- Buson, S -- Caliandro, G A -- Cameron, R A -- Caraveo, P A -- Casandjian, J M -- Cecchi, C -- Celik, O -- Charles, E -- Chaves, R C G -- Cheung, C C -- Chiang, J -- Ciprini, S -- Claus, R -- Cohen-Tanugi, J -- Conrad, J -- Cutini, S -- D'Ammando, F -- Dermer, C D -- Digel, S W -- Drell, P S -- Drlica-Wagner, A -- Dubois, R -- Dumora, D -- Favuzzi, C -- Ferrara, E C -- Franckowiak, A -- Fukazawa, Y -- Fusco, P -- Gargano, F -- Gehrels, N -- Germani, S -- Giglietto, N -- Giordano, F -- Giroletti, M -- Godfrey, G -- Grenier, I A -- Grondin, M-H -- Grove, J E -- Guiriec, S -- Hadasch, D -- Hanabata, Y -- Harding, A K -- den Hartog, P R -- Hayashida, M -- Hays, E -- Hill, A B -- Hou, X -- Hughes, R E -- Johannesson, G -- Jackson, M S -- Jogler, T -- Johnson, A S -- Johnson, W N -- Kataoka, J -- Kerr, M -- Knodlseder, J -- Kuss, M -- Lande, J -- Larsson, S -- Latronico, L -- Lemoine-Goumard, M -- Longo, F -- Loparco, F -- Lovellette, M N -- Lubrano, P -- Massaro, F -- Mayer, M -- Mazziotta, M N -- McEnery, J E -- Mehault, J -- Michelson, P F -- Mitthumsiri, W -- Mizuno, T -- Monzani, M E -- Morselli, A -- Moskalenko, I V -- Murgia, S -- Nakamori, T -- Nemmen, R -- Nuss, E -- Ohno, M -- Ohsugi, T -- Omodei, N -- Orienti, M -- Orlando, E -- de Palma, F -- Paneque, D -- Perkins, J S -- Piron, F -- Pivato, G -- Porter, T A -- Raino, S -- Rando, R -- Ray, P S -- Razzano, M -- Reimer, A -- Reimer, O -- Reposeur, T -- Ritz, S -- Romani, R W -- Romoli, C -- Sanchez, D A -- Saz Parkinson, P M -- Schulz, A -- Sgro, C -- do Couto e Silva, E -- Siskind, E J -- Smith, D A -- Spandre, G -- Spinelli, P -- Suson, D J -- Takahashi, H -- Tanaka, T -- Thayer, J B -- Thayer, J G -- Thompson, D J -- Tibaldo, L -- Tinivella, M -- Troja, E -- Usher, T L -- Vandenbroucke, J -- Vasileiou, V -- Vianello, G -- Vitale, V -- Waite, A P -- Winer, B L -- Wood, K S -- Wood, M -- Yang, Z -- Zimmer, S -- New York, N.Y. -- Science. 2012 Dec 7;338(6112):1314-7. doi: 10.1126/science.1229054. Epub 2012 Oct 25.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Max-Planck-Institut fur Gravitationsphysik (Albert-Einstein-Institut), D-30167 Hannover, Germany. holger.pletsch@aei.mpg.de〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23112297" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
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  • 5
    Publikationsdatum: 2012-08-31
    Beschreibung: We report the detection of Kepler-47, a system consisting of two planets orbiting around an eclipsing pair of stars. The inner and outer planets have radii 3.0 and 4.6 times that of Earth, respectively. The binary star consists of a Sun-like star and a companion roughly one-third its size, orbiting each other every 7.45 days. With an orbital period of 49.5 days, 18 transits of the inner planet have been observed, allowing a detailed characterization of its orbit and those of the stars. The outer planet's orbital period is 303.2 days, and although the planet is not Earth-like, it resides within the classical "habitable zone," where liquid water could exist on an Earth-like planet. With its two known planets, Kepler-47 establishes that close binary stars can host complete planetary systems.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Orosz, Jerome A -- Welsh, William F -- Carter, Joshua A -- Fabrycky, Daniel C -- Cochran, William D -- Endl, Michael -- Ford, Eric B -- Haghighipour, Nader -- MacQueen, Phillip J -- Mazeh, Tsevi -- Sanchis-Ojeda, Roberto -- Short, Donald R -- Torres, Guillermo -- Agol, Eric -- Buchhave, Lars A -- Doyle, Laurance R -- Isaacson, Howard -- Lissauer, Jack J -- Marcy, Geoffrey W -- Shporer, Avi -- Windmiller, Gur -- Barclay, Thomas -- Boss, Alan P -- Clarke, Bruce D -- Fortney, Jonathan -- Geary, John C -- Holman, Matthew J -- Huber, Daniel -- Jenkins, Jon M -- Kinemuchi, Karen -- Kruse, Ethan -- Ragozzine, Darin -- Sasselov, Dimitar -- Still, Martin -- Tenenbaum, Peter -- Uddin, Kamal -- Winn, Joshua N -- Koch, David G -- Borucki, William J -- New York, N.Y. -- Science. 2012 Sep 21;337(6101):1511-4. Epub 2012 Aug 28.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Astronomy Department, San Diego State University, 5500 Campanile Drive, San Diego, CA 92182, USA. orosz@sciences.sdsu.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22933522" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
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  • 6
    Publikationsdatum: 2012-06-30
    Beschreibung: Wood is a major pool of organic carbon that is highly resistant to decay, owing largely to the presence of lignin. The only organisms capable of substantial lignin decay are white rot fungi in the Agaricomycetes, which also contains non-lignin-degrading brown rot and ectomycorrhizal species. Comparative analyses of 31 fungal genomes (12 generated for this study) suggest that lignin-degrading peroxidases expanded in the lineage leading to the ancestor of the Agaricomycetes, which is reconstructed as a white rot species, and then contracted in parallel lineages leading to brown rot and mycorrhizal species. Molecular clock analyses suggest that the origin of lignin degradation might have coincided with the sharp decrease in the rate of organic carbon burial around the end of the Carboniferous period.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Floudas, Dimitrios -- Binder, Manfred -- Riley, Robert -- Barry, Kerrie -- Blanchette, Robert A -- Henrissat, Bernard -- Martinez, Angel T -- Otillar, Robert -- Spatafora, Joseph W -- Yadav, Jagjit S -- Aerts, Andrea -- Benoit, Isabelle -- Boyd, Alex -- Carlson, Alexis -- Copeland, Alex -- Coutinho, Pedro M -- de Vries, Ronald P -- Ferreira, Patricia -- Findley, Keisha -- Foster, Brian -- Gaskell, Jill -- Glotzer, Dylan -- Gorecki, Pawel -- Heitman, Joseph -- Hesse, Cedar -- Hori, Chiaki -- Igarashi, Kiyohiko -- Jurgens, Joel A -- Kallen, Nathan -- Kersten, Phil -- Kohler, Annegret -- Kues, Ursula -- Kumar, T K Arun -- Kuo, Alan -- LaButti, Kurt -- Larrondo, Luis F -- Lindquist, Erika -- Ling, Albee -- Lombard, Vincent -- Lucas, Susan -- Lundell, Taina -- Martin, Rachael -- McLaughlin, David J -- Morgenstern, Ingo -- Morin, Emanuelle -- Murat, Claude -- Nagy, Laszlo G -- Nolan, Matt -- Ohm, Robin A -- Patyshakuliyeva, Aleksandrina -- Rokas, Antonis -- Ruiz-Duenas, Francisco J -- Sabat, Grzegorz -- Salamov, Asaf -- Samejima, Masahiro -- Schmutz, Jeremy -- Slot, Jason C -- St John, Franz -- Stenlid, Jan -- Sun, Hui -- Sun, Sheng -- Syed, Khajamohiddin -- Tsang, Adrian -- Wiebenga, Ad -- Young, Darcy -- Pisabarro, Antonio -- Eastwood, Daniel C -- Martin, Francis -- Cullen, Dan -- Grigoriev, Igor V -- Hibbett, David S -- New York, N.Y. -- Science. 2012 Jun 29;336(6089):1715-9. doi: 10.1126/science.1221748.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Biology Department, Clark University, Worcester, MA 01610, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22745431" target="_blank"〉PubMed〈/a〉
    Schlagwort(e): Basidiomycota/classification/*enzymology/*genetics ; Bayes Theorem ; *Evolution, Molecular ; *Genome, Fungal ; Indoles ; Lignin/*metabolism ; Peroxidases/*genetics/metabolism ; Wood/metabolism
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
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  • 7
    Publikationsdatum: 2012-12-22
    Beschreibung: Doppler weather radar imaging enabled the rapid recovery of the Sutter's Mill meteorite after a rare 4-kiloton of TNT-equivalent asteroid impact over the foothills of the Sierra Nevada in northern California. The recovered meteorites survived a record high-speed entry of 28.6 kilometers per second from an orbit close to that of Jupiter-family comets (Tisserand's parameter = 2.8 +/- 0.3). Sutter's Mill is a regolith breccia composed of CM (Mighei)-type carbonaceous chondrite and highly reduced xenolithic materials. It exhibits considerable diversity of mineralogy, petrography, and isotope and organic chemistry, resulting from a complex formation history of the parent body surface. That diversity is quickly masked by alteration once in the terrestrial environment but will need to be considered when samples returned by missions to C-class asteroids are interpreted.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Jenniskens, Peter -- Fries, Marc D -- Yin, Qing-Zhu -- Zolensky, Michael -- Krot, Alexander N -- Sandford, Scott A -- Sears, Derek -- Beauford, Robert -- Ebel, Denton S -- Friedrich, Jon M -- Nagashima, Kazuhide -- Wimpenny, Josh -- Yamakawa, Akane -- Nishiizumi, Kunihiko -- Hamajima, Yasunori -- Caffee, Marc W -- Welten, Kees C -- Laubenstein, Matthias -- Davis, Andrew M -- Simon, Steven B -- Heck, Philipp R -- Young, Edward D -- Kohl, Issaku E -- Thiemens, Mark H -- Nunn, Morgan H -- Mikouchi, Takashi -- Hagiya, Kenji -- Ohsumi, Kazumasa -- Cahill, Thomas A -- Lawton, Jonathan A -- Barnes, David -- Steele, Andrew -- Rochette, Pierre -- Verosub, Kenneth L -- Gattacceca, Jerome -- Cooper, George -- Glavin, Daniel P -- Burton, Aaron S -- Dworkin, Jason P -- Elsila, Jamie E -- Pizzarello, Sandra -- Ogliore, Ryan -- Schmitt-Kopplin, Phillipe -- Harir, Mourad -- Hertkorn, Norbert -- Verchovsky, Alexander -- Grady, Monica -- Nagao, Keisuke -- Okazaki, Ryuji -- Takechi, Hiroyuki -- Hiroi, Takahiro -- Smith, Ken -- Silber, Elizabeth A -- Brown, Peter G -- Albers, Jim -- Klotz, Doug -- Hankey, Mike -- Matson, Robert -- Fries, Jeffrey A -- Walker, Richard J -- Puchtel, Igor -- Lee, Cin-Ty A -- Erdman, Monica E -- Eppich, Gary R -- Roeske, Sarah -- Gabelica, Zelimir -- Lerche, Michael -- Nuevo, Michel -- Girten, Beverly -- Worden, Simon P -- Sutter's Mill Meteorite Consortium -- New York, N.Y. -- Science. 2012 Dec 21;338(6114):1583-7. doi: 10.1126/science.1227163.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉SETI Institute, Mountain View, CA 94043, USA. petrus.m.jenniskens@nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23258889" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
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  • 8
    Publikationsdatum: 2012-08-28
    Beschreibung: There is a consensus that type Ia supernovae (SNe Ia) arise from the thermonuclear explosion of white dwarf stars that accrete matter from a binary companion. However, direct observation of SN Ia progenitors is lacking, and the precise nature of the binary companion remains uncertain. A temporal series of high-resolution optical spectra of the SN Ia PTF 11kx reveals a complex circumstellar environment that provides an unprecedentedly detailed view of the progenitor system. Multiple shells of circumstellar material are detected, and the SN ejecta are seen to interact with circumstellar material starting 59 days after the explosion. These features are best described by a symbiotic nova progenitor, similar to RS Ophiuchi.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Dilday, B -- Howell, D A -- Cenko, S B -- Silverman, J M -- Nugent, P E -- Sullivan, M -- Ben-Ami, S -- Bildsten, L -- Bolte, M -- Endl, M -- Filippenko, A V -- Gnat, O -- Horesh, A -- Hsiao, E -- Kasliwal, M M -- Kirkman, D -- Maguire, K -- Marcy, G W -- Moore, K -- Pan, Y -- Parrent, J T -- Podsiadlowski, P -- Quimby, R M -- Sternberg, A -- Suzuki, N -- Tytler, D R -- Xu, D -- Bloom, J S -- Gal-Yam, A -- Hook, I M -- Kulkarni, S R -- Law, N M -- Ofek, E O -- Polishook, D -- Poznanski, D -- New York, N.Y. -- Science. 2012 Aug 24;337(6097):942-5. doi: 10.1126/science.1219164.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Las Cumbres Observatory Global Telescope Network, 6740 Cortona Drive, Suite 102, Goleta, CA 93117, USA. bdilday@lcogt.net〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22923575" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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  • 9
    Publikationsdatum: 2012-05-15
    Beschreibung: Vesta's surface is characterized by abundant impact craters, some with preserved ejecta blankets, large troughs extending around the equatorial region, enigmatic dark material, and widespread mass wasting, but as yet an absence of volcanic features. Abundant steep slopes indicate that impact-generated surface regolith is underlain by bedrock. Dawn observations confirm the large impact basin (Rheasilvia) at Vesta's south pole and reveal evidence for an earlier, underlying large basin (Veneneia). Vesta's geology displays morphological features characteristic of the Moon and terrestrial planets as well as those of other asteroids, underscoring Vesta's unique role as a transitional solar system body.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Jaumann, R -- Williams, D A -- Buczkowski, D L -- Yingst, R A -- Preusker, F -- Hiesinger, H -- Schmedemann, N -- Kneissl, T -- Vincent, J B -- Blewett, D T -- Buratti, B J -- Carsenty, U -- Denevi, B W -- De Sanctis, M C -- Garry, W B -- Keller, H U -- Kersten, E -- Krohn, K -- Li, J-Y -- Marchi, S -- Matz, K D -- McCord, T B -- McSween, H Y -- Mest, S C -- Mittlefehldt, D W -- Mottola, S -- Nathues, A -- Neukum, G -- O'Brien, D P -- Pieters, C M -- Prettyman, T H -- Raymond, C A -- Roatsch, T -- Russell, C T -- Schenk, P -- Schmidt, B E -- Scholten, F -- Stephan, K -- Sykes, M V -- Tricarico, P -- Wagner, R -- Zuber, M T -- Sierks, H -- New York, N.Y. -- Science. 2012 May 11;336(6082):687-90. doi: 10.1126/science.1219122.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉German Aerospace Center, Institute of Planetary Research, Berlin, Germany. ralf.jaumann@dlr.de〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22582254" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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  • 10
    Publikationsdatum: 2012-07-17
    Beschreibung: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Chown, S L -- Lee, J E -- Hughes, K A -- Barnes, J -- Barrett, P J -- Bergstrom, D M -- Convey, P -- Cowan, D A -- Crosbie, K -- Dyer, G -- Frenot, Y -- Grant, S M -- Herr, D -- Kennicutt, M C 2nd -- Lamers, M -- Murray, A -- Possingham, H P -- Reid, K -- Riddle, M J -- Ryan, P G -- Sanson, L -- Shaw, J D -- Sparrow, M D -- Summerhayes, C -- Terauds, A -- Wall, D H -- New York, N.Y. -- Science. 2012 Jul 13;337(6091):158-9. doi: 10.1126/science.1222821.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Centre for Invasion Biology, Stellenbosch University, Matieland, South Africa. steven.chown@monash.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22798586" target="_blank"〉PubMed〈/a〉
    Schlagwort(e): Animals ; Antarctic Regions ; Climate Change ; *Conservation of Natural Resources/trends ; *Ecosystem ; Forecasting ; Human Activities ; Humans ; Public Policy ; Travel
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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