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Long γ-ray bursts and core-collapse supernovae have different environments

Author
FRUCHTER, A. S1 ; LEVAN, A. J1 2 3 ; DAHLEN, T13 ; FERGUSON, H. C1 ; FYNBO, J. P. U9 ; GARNAVICH, P. M14 ; GIBBONS, R. A1 15 ; GOROSABE, J1 10 ; GULL, T. R16 ; HJORTH, J9 ; HOLLAND, S. T17 ; KOUVELIOTOU, C18 ; STROLGER, L1 4 ; LEVAY, Z1 ; LIVIO, M1 ; METZGER, M. R19 ; NUGENT, P. E20 ; PETRO, L1 ; PIAN, E21 ; RHOADS, J. E1 ; RIESS, A. G1 ; SAHU, K. C1 ; SMETTE, A5 ; VREESWIJK, P. M5 ; TANVIR, N. R3 ; WIJERS, R. A. M. J22 ; WOOSLEY, S. E6 ; THORSETT, S. E6 ; BERSIER, D1 7 ; BURUD, I1 8 ; CASTRO CERON, J. M1 9 ; CASTRO-TIRADO, A. J10 ; CONSELICE, C11 12
[1] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, United States
[2] Department of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, United Kingdom
[3] Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, AL10 9AB, United Kingdom
[4] Physics & Astronomy, TCCW 246, Western Kentucky University, 1 Big Red Way, Bowling Green, Kentucky 42101, United States
[5] European Southern Observatory, Alonso de C6rdova 3107, Casilla 19001, Santiago, Chile
[6] Department of Astronomy & Astrophysics, University of California, 1156 High Street, Santa Cruz, California 95064, United States
[7] Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead, CH411LD, United Kingdom
[8] Norwegian Meteorological Institute, PO Box 43, Blindern, 0313 Oslo, Norway
[9] Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, 2100 Copenhagen, Denmark
[10] Instituto de Astrofisica de Andalucía (CSIC), Camino Bajo de Huetor, 50, 18008 Granada, Spain
[11] California Institute of Technology, Mail Code 105-24, Pasadena, California 91125, United States
[12] School of Physics and Astronomy, University of Nottingham, University Park, Nottingham, NG7 2RD, United Kingdom
[13] Department of Physics, Stockholm University, 106 91 Stockholm, Sweden
[14] Physics Department, University of Notre Dame, 225 Nieuwland Hall, Notre Dame, Indiana 46556, United States
[15] Vanderbilt University, Department of Physics and Astronomy, 6301 Stevenson Center, Nashville, Tennessee 37235, United States
[16] Code 667, Extraterrestial Planets and Stellar Astrophysics, Exploration of the Universe Division, United States
[17] Code 6601, Goddard Space Flight Center, Greenbelt, Maryland 20771, United States
[18] NASA/Marshall Space Flight Center, VP-62, National Space Science & Technology Center, 320 Sparkman Drive, Huntsville, Alabama 35805, United States
[19] Renaissance Technologies Corporation, 600 Route 25A, East Setauket, New York 11733, United States
[20] Lawrence Berkeley National Laboratory, MS 50F-1650,1 Cyclotron Road, Berkeley, California 94720, United States
[21] INAF, Osservatorio Astronomico di Trieste, Via G B Tiepolo 11, 34131 Trieste, Italy
[22] Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, Netherlands
Source

Nature (London). 2006, Vol 441, Num 7092, pp 463-468, 6 p ; ref : 50 ref

CODEN
NATUAS
ISSN
0028-0836
Scientific domain
Multidisciplinary
Publisher
Nature Publishing, London
Publication country
United Kingdom
Document type
Article
Language
English
Keyword (fr)
Effondrement Etoile massive Evolution chimique Galaxies Source gamma cosmique Supernova Sursaut Rγ Sursaut gamma cosmique Voie lactée
Keyword (en)
Collapse Massive stars Chemical evolution Galaxies Cosmic gamma sources Supernovae Gamma ray burst Cosmic gamma bursts Milky Way
Keyword (es)
Desmoronamiento Evolución química Arrebato Rγ
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D70 Unidentified sources and radiation outside the solar system / 001E03D70R Gamma-ray sources ; gamma-ray bursts

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
17778189

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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