Search Results - (Author, Cooperation:D. C. Leonard)
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1A. Sternberg ; A. Gal-Yam ; J. D. Simon ; D. C. Leonard ; R. M. Quimby ; M. M. Phillips ; N. Morrell ; I. B. Thompson ; I. Ivans ; J. L. Marshall ; A. V. Filippenko ; G. W. Marcy ; J. S. Bloom ; F. Patat ; R. J. Foley ; D. Yong ; B. E. Penprase ; D. J. Beeler ; C. Allende Prieto ; G. S. Stringfellow
American Association for the Advancement of Science (AAAS)
Published 2011Staff ViewPublication Date: 2011-08-13Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Fox, D. B. ; Price, P. A. ; Ofek, E. O. ; Davis, M. R. ; Leonard, D. C. ; Soderberg, A. M. ; Schmidt, B. P. ; Lewis, K. M. ; Peterson, B. A. ; Kulkarni, S. R. ; Berger, E. ; Cenko, S. B. ; Sari, R. ; Sharon, K. ; Frail, D. ; Moon, D.-S. ; Brown, P. J. ; Cucchiara, A. ; Harrison, F. ; Piran, T. ; Persson, S. E. ; McCarthy, P. J. ; Penprase, B. E. ; Chevalier, R. A. ; MacFadyen, A. I.
[s.l.] : Nature Publishing Group
Published 2006Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Over the past decade, our physical understanding of γ-ray bursts (GRBs) has progressed rapidly, thanks to the discovery and observation of their long-lived afterglow emission. Long-duration (≳2 s) GRBs are associated with the explosive deaths of massive stars ...Type of Medium: Electronic ResourceURL: -
3Price, P. A. ; Cenko, S. B. ; Gal-Yam, A. ; Soderberg, A. M. ; Kasliwal, M. ; Leonard, D. C. ; Cameron, P. B. ; Frail, D. A. ; Kulkarni, S. R. ; Murphy, D. C. ; Krzeminski, W. ; Piran, T. ; Lee, B. L. ; Roth, K. C. ; Moon, D.-S. ; Fox, D. B. ; Harrison, F. A. ; Persson, S. E. ; Schmidt, B. P. ; Penprase, B. E. ; Rich, J. ; Peterson, B. A. ; Cowie, L. L. ; Berger, E.
[s.l.] : Nature Publishing Group
Published 2005Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Despite a rich phenomenology, γ-ray bursts (GRBs) are divided into two classes based on their duration and spectral hardness—the long-soft and the short-hard bursts. The discovery of afterglow emission from long GRBs was a watershed event, pinpointing their origin to star-forming ...Type of Medium: Electronic ResourceURL: -
4Kulkarni, S. R. ; Djorgovski, S. G. ; Eichelberger, A. C. ; Côté, P. ; Blakeslee, J. P. ; Odewahn, S. C. ; Harrison, F. A. ; Frail, D. A. ; Filippenko, A. V. ; Leonard, D. C. ; Riess, A. G. ; Spinrad, H. ; Stern, D. ; Bunker, A. ; Dey, A. ; Grossan, B. ; Perlmutter, S. ; Knop, R. A. ; Hook, I. M. ; Feroci, M. ; Bloom, J. S.
[s.l.] : Macmillian Magazines Ltd.
Published 1999Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Cosmic γ-ray bursts have now been firmly established as one of the most powerful phenomena in the Universe, releasing almost the rest-mass energy of a neutron star within the space of a few seconds (ref. 1). The two most popular models to explain γ-ray bursts are ...Type of Medium: Electronic ResourceURL: