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  • 1
    Publication Date: 2014-10-22
    Description: Wind turbines are causing unprecedented numbers of bat fatalities. Many fatalities involve tree-roosting bats, but reasons for this higher susceptibility remain unknown. To better understand behaviors associated with risk, we monitored bats at three experimentally manipulated wind turbines in Indiana, United States, from July 29 to October 1, 2012, using...
    Print ISSN: 0027-8424
    Electronic ISSN: 1091-6490
    Topics: Biology , Medicine , Natural Sciences in General
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  • 2
    Publication Date: 2012-07-12
    Description: The Journal of Physical Chemistry B DOI: 10.1021/jp304018b
    Electronic ISSN: 1520-5207
    Topics: Chemistry and Pharmacology , Physics
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  • 3
    Publication Date: 2011-09-30
    Description: Author(s): N. Prantzos, C. Boehm, A. M. Bykov, R. Diehl, K. Ferrière, N. Guessoum, P. Jean, J. Knoedlseder, A. Marcowith, I. V. Moskalenko, A. Strong, and G. Weidenspointner The first gamma-ray line ever detected from outside the Solar System witnesses electron-positron annihilation in the Galaxy. Its true origin is still not understood but after 30 years of research, gamma-ray observatories revealed a strong concentration of the emission towards the galactic bulge with... [Rev. Mod. Phys. 83, 1001] Published Thu Sep 29, 2011
    Keywords: Astrophysics
    Print ISSN: 0034-6861
    Electronic ISSN: 1539-0756
    Topics: Physics
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  • 4
    Publication Date: 2008-01-11
    Description: Gamma-ray line radiation at 511 keV is the signature of electron-positron annihilation. Such radiation has been known for 30 years to come from the general direction of the Galactic Centre, but the origin of the positrons has remained a mystery. Stellar nucleosynthesis, accreting compact objects, and even the annihilation of exotic dark-matter particles have all been suggested. Here we report a distinct asymmetry in the 511-keV line emission coming from the inner Galactic disk ( approximately 10-50 degrees from the Galactic Centre). This asymmetry resembles an asymmetry in the distribution of low mass X-ray binaries with strong emission at photon energies 〉20 keV ('hard' LMXBs), indicating that they may be the dominant origin of the positrons. Although it had long been suspected that electron-positron pair plasmas may exist in X-ray binaries, it was not evident that many of the positrons could escape to lose energy and ultimately annihilate with electrons in the interstellar medium and thus lead to the emission of a narrow 511-keV line. For these models, our result implies that up to a few times 10(41) positrons escape per second from a typical hard LMXB. Positron production at this level from hard LMXBs in the Galactic bulge would reduce (and possibly eliminate) the need for more exotic explanations, such as those involving dark matter.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Weidenspointner, Georg -- Skinner, Gerry -- Jean, Pierre -- Knodlseder, Jurgen -- von Ballmoos, Peter -- Bignami, Giovanni -- Diehl, Roland -- Strong, Andrew W -- Cordier, Bertrand -- Schanne, Stephane -- Winkler, Christoph -- England -- Nature. 2008 Jan 10;451(7175):159-62. doi: 10.1038/nature06490.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Centre d'Etude Spatiale des Rayonnements, CNRS/UPS, BP 44346, Toulouse Cedex 4, France. Georg.Weidenspointner@hll.mpg.de〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/18185581" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 5
    Publication Date: 2015-07-15
    Description: A new class of ultra-long-duration (more than 10,000 seconds) gamma-ray bursts has recently been suggested. They may originate in the explosion of stars with much larger radii than those producing normal long-duration gamma-ray bursts or in the tidal disruption of a star. No clear supernova has yet been associated with an ultra-long-duration gamma-ray burst. Here we report that a supernova (SN 2011kl) was associated with the ultra-long-duration gamma-ray burst GRB 111209A, at a redshift z of 0.677. This supernova is more than three times more luminous than type Ic supernovae associated with long-duration gamma-ray bursts, and its spectrum is distinctly different. The slope of the continuum resembles those of super-luminous supernovae, but extends further down into the rest-frame ultraviolet implying a low metal content. The light curve evolves much more rapidly than those of super-luminous supernovae. This combination of high luminosity and low metal-line opacity cannot be reconciled with typical type Ic supernovae, but can be reproduced by a model where extra energy is injected by a strongly magnetized neutron star (a magnetar), which has also been proposed as the explanation for super-luminous supernovae.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Greiner, Jochen -- Mazzali, Paolo A -- Kann, D Alexander -- Kruhler, Thomas -- Pian, Elena -- Prentice, Simon -- Olivares E, Felipe -- Rossi, Andrea -- Klose, Sylvio -- Taubenberger, Stefan -- Knust, Fabian -- Afonso, Paulo M J -- Ashall, Chris -- Bolmer, Jan -- Delvaux, Corentin -- Diehl, Roland -- Elliott, Jonathan -- Filgas, Robert -- Fynbo, Johan P U -- Graham, John F -- Guelbenzu, Ana Nicuesa -- Kobayashi, Shiho -- Leloudas, Giorgos -- Savaglio, Sandra -- Schady, Patricia -- Schmidl, Sebastian -- Schweyer, Tassilo -- Sudilovsky, Vladimir -- Tanga, Mohit -- Updike, Adria C -- van Eerten, Hendrik -- Varela, Karla -- England -- Nature. 2015 Jul 9;523(7559):189-92. doi: 10.1038/nature14579.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉1] Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany [2] Excellence Cluster Universe, Technische Universitat Munchen, Boltzmannstrasse 2, 85748 Garching, Germany. ; 1] Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Browlow Hill, Liverpool L3 5RF, UK [2] Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany. ; 1] Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany [2] Excellence Cluster Universe, Technische Universitat Munchen, Boltzmannstrasse 2, 85748 Garching, Germany [3] Thuringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany. ; European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago 19, Chile. ; 1] INAF, Institute of Space Astrophysics and Cosmic Physics, via P. Gobetti 101, 40129 Bologna, Italy [2] Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy. ; Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Browlow Hill, Liverpool L3 5RF, UK. ; Departamento de Ciencias Fisicas, Universidad Andres Bello, Avenida Republica 252, Santiago, Chile. ; 1] Thuringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany [2] INAF, Institute of Space Astrophysics and Cosmic Physics, via P. Gobetti 101, 40129 Bologna, Italy. ; Thuringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany. ; 1] Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany [2] European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany. ; Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany. ; American River College, Physics and Astronomy Department, 4700 College Oak Drive, Sacramento, California 95841, USA. ; 1] Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany [2] Technische Universitat Munchen, Physik Department, James-Franck-Strasse, 85748 Garching, Germany. ; 1] Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany [2] Astrophysics Data System, Harvard-Smithonian Center for Astrophysics, Garden Street 60, Cambridge, Massachusetts 02138, USA. ; Institute of Experimental and Applied Physics, Czech Technical University in Prague, Horska 3a/22, 128 00 Prague 2, Czech Republic. ; DARK Cosmology Center, Niels-Bohr-Institut, University of Copenhagen, Juliane Maries Vej 30, 2100 Kobenhavn, Denmark. ; 1] DARK Cosmology Center, Niels-Bohr-Institut, University of Copenhagen, Juliane Maries Vej 30, 2100 Kobenhavn, Denmark [2] Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 76100, Israel. ; 1] Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany [2] Universita della Calabria, 87036 Arcavacata di Rende, via P. Bucci, Italy. ; Roger Williams University, 1 Old Ferry Road, Bristol, Rhode Island 02809, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/26156372" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 6
    Publication Date: 2006-03-11
    Description: A biosynthetic approach was developed to control and probe cooperativity in multiunit biomotor assemblies by linking molecular motors to artificial protein scaffolds. This approach provides precise control over spatial and elastic coupling between motors. Cooperative interactions between monomeric kinesin-1 motors attached to protein scaffolds enhance hydrolysis activity and microtubule gliding velocity. However, these interactions are not influenced by changes in the elastic properties of the scaffold, distinguishing multimotor transport from that powered by unorganized monomeric motors. These results highlight the role of supramolecular architecture in determining mechanisms of collective transport.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Diehl, Michael R -- Zhang, Kechun -- Lee, Heun Jin -- Tirrell, David A -- New York, N.Y. -- Science. 2006 Mar 10;311(5766):1468-71.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA 91125, USA. diehl@rice.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/16527982" target="_blank"〉PubMed〈/a〉
    Keywords: Adenosine Triphosphatases/chemistry ; Amino Acid Sequence ; Elasticity ; Elastin/chemistry ; Hydrolysis ; Kinesin/chemistry ; Microtubules/physiology ; Models, Biological ; Molecular Motor Proteins/*physiology ; Molecular Sequence Data ; Protein Engineering ; Protein Structure, Tertiary ; Proteins/chemistry/*physiology ; Recombinant Proteins/chemistry ; Structure-Activity Relationship
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 7
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2012-11-03
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Diehl, Michael R -- New York, N.Y. -- Science. 2012 Nov 2;338(6107):626-7. doi: 10.1126/science.1230818.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Chemistry, Rice University, Houston, TX 77030, USA. diehl@rice.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23118181" target="_blank"〉PubMed〈/a〉
    Keywords: Cytoplasmic Dyneins/*metabolism ; DNA/*chemistry/*metabolism ; Kinesin/*metabolism ; Microtubules/*metabolism ; Molecular Motor Proteins/*metabolism
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 8
    Publication Date: 2018-11-14
    Description: A wide range of mutations in the kinesin motor Kif5A have been linked to a neuronal disorder called hereditary spastic paraplegia (HSP). The position of these mutations can vary, and a range of different motile behaviors have been observed, indicating that the HSP mutants can alter distinct aspects of kinesin...
    Print ISSN: 0027-8424
    Electronic ISSN: 1091-6490
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  • 9
    Publication Date: 2014-08-02
    Description: Type Ia supernovae result from binary systems that include a carbon-oxygen white dwarf, and these thermonuclear explosions typically produce 0.5 solar mass of radioactive (56)Ni. The (56)Ni is commonly believed to be buried deeply in the expanding supernova cloud. In SN2014J, we detected the lines at 158 and 812 kiloelectron volts from (56)Ni decay (time ~8.8 days) earlier than the expected several-week time scale, only ~20 days after the explosion and with flux levels corresponding to roughly 10% of the total expected amount of (56)Ni. Some mechanism must break the spherical symmetry of the supernova and at the same time create a major amount of (56)Ni at the outskirts. A plausible explanation is that a belt of helium from the companion star is accreted by the white dwarf, where this material explodes and then triggers the supernova event.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Diehl, Roland -- Siegert, Thomas -- Hillebrandt, Wolfgang -- Grebenev, Sergei A -- Greiner, Jochen -- Krause, Martin -- Kromer, Markus -- Maeda, Keiichi -- Ropke, Friedrich -- Taubenberger, Stefan -- New York, N.Y. -- Science. 2014 Sep 5;345(6201):1162-5. doi: 10.1126/science.1254738. Epub 2014 Jul 31.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, D-85741 Garching, Germany rod@mpe.mpg.de. ; Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, D-85741 Garching, Germany. ; Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany. ; Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia. ; The Oskar Klein Centre and Department of Astronomy, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden. ; Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502, and Kavli Institute (WPI), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan. ; Institut fur Theoretische Physik und Astrophysik, Universitat Wurzburg, Emil-Fischer-Strasse 31, 97074 Wurzburg, Germany.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25081484" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 10
    Publication Date: 2017-10-11
    Description: Motor proteins are active enzymatic molecules that support important cellular processes by transforming chemical energy into mechanical work. Although the structures and chemomechanical cycles of motor proteins have been extensively investigated, the sensitivity of a motor’s velocity in response to a force is not well-understood. For kinesin, velocity is weakly...
    Print ISSN: 0027-8424
    Electronic ISSN: 1091-6490
    Topics: Biology , Medicine , Natural Sciences in General
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