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  • American Association for the Advancement of Science (AAAS)  (2)
  • 2005-2009  (2)
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  • 1
    Publication Date: 2006-06-10
    Description: We present late-time optical and mid-infrared observations of the Type II supernova 2003gd in the galaxy NGC 628. Mid-infrared excesses consistent with cooling dust in the ejecta are observed 499 to 678 days after outburst and are accompanied by increasing optical extinction and growing asymmetries in the emission-line profiles. Radiative-transfer models show that up to 0.02 solar masses of dust has formed within the ejecta, beginning as early as 250 days after outburst. These observations show that dust formation in supernova ejecta can be efficient and that massive-star supernovae could have been major dust producers throughout the history of the universe.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Sugerman, Ben E K -- Ercolano, Barbara -- Barlow, M J -- Tielens, A G G M -- Clayton, Geoffrey C -- Zijlstra, Albert A -- Meixner, Margaret -- Speck, Angela -- Gledhill, Tim M -- Panagia, Nino -- Cohen, Martin -- Gordon, Karl D -- Meyer, Martin -- Fabbri, Joanna -- Bowey, Janet E -- Welch, Douglas L -- Regan, Michael W -- Kennicutt, Robert C Jr -- New York, N.Y. -- Science. 2006 Jul 14;313(5784):196-200. Epub 2006 Jun 8.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. sugerman@stsci.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/16763110" 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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  • 2
    Publication Date: 2008-07-26
    Description: The only supernovae (SNe) to show gamma-ray bursts (GRBs) or early x-ray emission thus far are overenergetic, broad-lined type Ic SNe (hypernovae, HNe). Recently, SN 2008D has shown several unusual features: (i) weak x-ray flash (XRF), (ii) an early, narrow optical peak, (iii) disappearance of the broad lines typical of SN Ic HNe, and (iv) development of helium lines as in SNe Ib. Detailed analysis shows that SN 2008D was not a normal supernova: Its explosion energy (E approximately 6x10(51) erg) and ejected mass [ approximately 7 times the mass of the Sun (M(middle dot in circle))] are intermediate between normal SNe Ibc and HNe. We conclude that SN 2008D was originally a approximately 30 M(middle dot in circle) star. When it collapsed, a black hole formed and a weak, mildly relativistic jet was produced, which caused the XRF. SN 2008D is probably among the weakest explosions that produce relativistic jets. Inner engine activity appears to be present whenever massive stars collapse to black holes.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Mazzali, Paolo A -- Valenti, Stefano -- Della Valle, Massimo -- Chincarini, Guido -- Sauer, Daniel N -- Benetti, Stefano -- Pian, Elena -- Piran, Tsvi -- D'Elia, Valerio -- Elias-Rosa, Nancy -- Margutti, Raffaella -- Pasotti, Francesco -- Antonelli, L Angelo -- Bufano, Filomena -- Campana, Sergio -- Cappellaro, Enrico -- Covino, Stefano -- D'Avanzo, Paolo -- Fiore, Fabrizio -- Fugazza, Dino -- Gilmozzi, Roberto -- Hunter, Deborah -- Maguire, Kate -- Maiorano, Elisabetta -- Marziani, Paola -- Masetti, Nicola -- Mirabel, Felix -- Navasardyan, Hripsime -- Nomoto, Ken'ichi -- Palazzi, Eliana -- Pastorello, Andrea -- Panagia, Nino -- Pellizza, L J -- Sari, Re'em -- Smartt, Stephen -- Tagliaferri, Gianpiero -- Tanaka, Masaomi -- Taubenberger, Stefan -- Tominaga, Nozomu -- Trundle, Carrie -- Turatto, Massimo -- New York, N.Y. -- Science. 2008 Aug 29;321(5893):1185-8. doi: 10.1126/science.1158088. Epub 2008 Jul 24.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Max-Planck Institut fur Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany. mazzali@mpa-garching.mpg.de〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/18653846" 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
    Location Call Number Expected Availability
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