DISENTANGLING THE ORIGIN AND HEATING MECHANISM OF SUPERNOVA DUST: LATE-TIME SPITZER SPECTROSCOPY OF THE TYPE IIn SN 2005ip

Record Type
Journal Articles
Full Title
DISENTANGLING THE ORIGIN AND HEATING MECHANISM OF SUPERNOVA DUST: LATE-TIME SPITZER SPECTROSCOPY OF THE TYPE IIn SN 2005ip
Author(s)
Fox O, Chevalier R, Dwek E, Skrutskie M, Sugerman B, Leisenring J
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2010 Dec
DOI
10.1088/0004-637X/725/2/1768
ISSN
0004-637X
Volume
725
Issue
2
Page Count
11
First Page
1768
Last Page
1778
Keyword(s)
Astronomy & Astrophysics, circumstellar matter, dust, extinction, infrared: stars, supernovae: general, supernovae: individual (SN 2005ip), LUMINOUS BLUE VARIABLES, INFRARED-EMISSION, SPACE-TELESCOPE, CIRCUMSTELLAR MEDIUM, MASSIVE STARS, SPECTROGRAPH, EJECTA, PROGENITORS, OUTBURST, 1987A
Citation
Fox O, Chevalier R, Dwek E, Skrutskie M, Sugerman B, Leisenring J. DISENTANGLING THE ORIGIN AND HEATING MECHANISM OF SUPERNOVA DUST: LATE-TIME SPITZER SPECTROSCOPY OF THE TYPE IIn SN 2005ip. ASTROPHYS J. 2010;725 (2):1768-1778.
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