THE PROPERTIES OF THE 2175 Å EXTINCTION FEATURE DISCOVERED IN GRB AFTERGLOWS
- Author
- ZAFAR, Tayyaba1 2 ; WATSON, Darach1 ; MORGAN, Adam N6 ; BLOOM, Joshua6 ; GREINER, Jochen3 ; ELIASDOTTIR, Ardís1 ; FYNBO, Johan P. U1 ; KRÜHLER, Thomas1 3 ; SCHADY, Patricia3 ; LELOUDAS, Giorgos1 ; JAKOBSSON, Páll4 ; THÖNE, Christina C5 ; PERLEY, Daniel A6
[1] Dark Cosmology Centre. Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
[2] Laboratoire d'Astrophysique de Marseille - LAM, Université Aix-Marseille & CNRS, UMR7326. 38 rue F. Joliot-Curie, 13388 Marseille, France
[3] Max-Planck Institut für Extraterrestrische Physik, Giessenbachstrasse, 85748. Garching, Germany
[4] Centre for Astrophysics and Cosmology, Science Institute. University of Iceland. Dunhagi 5, 107 Reykjavík, Iceland
[5] INAF-Osservatorio Astronomico di Brera, Via Bianchi 46, 23807, Merate (Lc), Italy
[6] Department of Astronomy, University of California, Berkeley. CA 94720-3411, United States - Source
The Astrophysical journal. 2012, Vol 753, Num 1 ; 82.1-82.9 ; 1 ; ref : 3/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- IOP, Bristol
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- dust, extinction gamma-ray burst: general gamma-ray burst: individual (GRB 080605, GRB 080805)
- Keyword (fr)
- Courbe extinction Densité spectrale énergie Groupe local Loi puissance Modèle Petit Nuage Magellan Position Postluminescence Source gamma cosmique Spectre optique Sursaut Rγ Voie lactée
- Keyword (en)
- Extinction curve Spectral energy distribution Local group Power law Models Small Magellanic Cloud Positions Afterglow Cosmic gamma sources Optical spectrum Gamma ray burst Milky Way
- Keyword (es)
- Curva extinción Densidad espectral energía Ley poder Modelo Espectro óptico Arrebato Rγ
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26821767
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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DOI
10.1088/0004-637X/753/1/82 
https://dx.doi.org/10.1088/0004-637X/753/1/82
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