Massive-star supernovae as major dust factories

Science

Volumn 313, Issue 5784, 2006, Pages 196-200

  Sugerman, Ben E K ^a   Ercolano, Barbara ^b   Barlow, M J ^b   Tielens, A G G M ^c   Clayton, Geoffrey C ^d   Zijlstra, Albert A ^e   Meixner, Margaret ^a   Speck, Angela ^f   Gledhill, Tim M ^g   Panagia, Nino ^a   Cohen, Martin ^h   Gordon, Karl D ⁱ   Meyer, Martin ^a   Fabbri, Joanna ^b   Bowey, Janet E ^b   Welch, Douglas L ^j   Regan, Michael W ^a   Kennicutt Jr , Robert C ^k  

^a AURA for the European Space Agency   (United States)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

^c UNIVERSITY OF GRONINGEN   (Netherlands)

^d LOUISIANA STATE UNIVERSITY   (United States)

^e UNIVERSITY OF MANCHESTER   (United Kingdom)

^f UNIVERSITY OF MISSOURI   (United States)

^g UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^h Monterey Institute for Research in Astronomy   (United States)

ⁱ UNIVERSITY OF ARIZONA   (United States)

^j MCMASTER UNIVERSITY   (Canada)

^k UNIVERSITY OF CAMBRIDGE   (United Kingdom)

more..

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; COOLING; LIGHT EXTINCTION; RADIATION;

GALAXY NGC 628; RADIATIVE-TRANSFER MODELS; SOLAR MASSES; TYPE II SUPERNOVA 2003GD;

GALAXIES;

ISOTOPE;

INTERPLANETARY DUST; OBSERVATIONAL METHOD;

ARTICLE; ASTRONOMY; COOLING; COSMOLOGICAL PHENOMENA; COSMOS; EXPLOSION; HYDRODYNAMICS; INFRARED RADIATION; OBSERVATION; OPTICAL INSTRUMENTATION; PHOTOMETRY; PRIORITY JOURNAL; RADIATION DETECTION; SIMULATION; SPECTROMETER; SPECTROSCOPY; SUPERNOVA; TIME;

EID: 33745983860     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1128131     Document Type: Article

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39. We gratefully acknowledge M. Hendry for providing optical spectra of SN 2003gd, and E. Dwek and P. Ghavamian for useful discussions. This work is based in part on archival data obtained with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA; with the NASA/European Space Agency Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc. (AURA), under NASA contract NAS 5-26555; and on observations obtained during the program GN-2004B-C-3 at the Gemini Observatory, which is operated by AURA under a cooperative agreement with the NSF on behalf of the Gemini partnership. Support for B.E.K.S. for this work was provided by Spitzer Space Telescope award GO-20320 issued by the Jet Propulsion Laboratory/ California Institute of Technology (JPL/Caltech). D.L.W. acknowledges support from the Natural Sciences and Engineering Research Council of Canada. M.C.'s participation was supported by JPL contract 1269553 with the Monterey Institute for Research in Astronomy.