INVERSE COMPTON X-RAY EMISSION FROM SUPERNOVAE WITH COMPACT PROGENITORS: APPLICATION TO SN2011fe

Record Type
Journal Articles
Full Title
INVERSE COMPTON X-RAY EMISSION FROM SUPERNOVAE WITH COMPACT PROGENITORS: APPLICATION TO SN2011fe
Author(s)
Margutti R, Soderberg A, Chomiuk L, Chevalier R, Hurley K, Milisavljevic D, Foley R, Hughes J, Slane P, Fransson C, Moe M, Barthelmy S, Boynton W, Briggs M, Connaughton V, Costa E, Cummings J, Del Monte E, Enos H, Fellows C, Feroci M, Fukazawa Y, Gehrels N, Goldsten J, Golovin D, Hanabata Y, Harshman K, Krimm H, Litvak M, Makishima K, Marisaldi M, Mitrofanov I, Murakami T, Ohno M, Palmer D, Sanin A, Starr R, Svinkin D, Takahashi T, Tashiro M, Terada Y, Yamaoka K
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2012 Jun 1
DOI
10.1088/0004-637X/751/2/134
ISSN
0004-637X
Volume
751
Issue
2
Page Count
10
Article Number
134
Keyword(s)
Astronomy & Astrophysics, radiation mechanisms: non-thermal, supernovae: individual (SN2011fe), SWIFT ULTRAVIOLET/OPTICAL TELESCOPE, SYMBIOTIC-STAR PROGENITOR, WHITE-DWARF MODELS, IA SUPERNOVAE, RADIO-EMISSION, LIGHT CURVES, SN 2011FE, CIRCUMSTELLAR MATERIAL, SODIUM-ABSORPTION, BURST AFTERGLOWS
Citation
Margutti R, Soderberg A, Chomiuk L, Chevalier R, Hurley K, Milisavljevic D, Foley R, Hughes J, Slane P, Fransson C, et al. INVERSE COMPTON X-RAY EMISSION FROM SUPERNOVAE WITH COMPACT PROGENITORS: APPLICATION TO SN2011fe. ASTROPHYS J. 2012;751 (2):10.
Conditions of Use
  • Author can archive pre-print (i.e., pre-refereeing)
  • Author can archive post-print (i.e., final draft post-refereeing)
  • On any website or open access repository
  • Publisher copyright and source must be acknowledged
  • Must link to publisher version
  • Publisher's version/PDF may be used

More usage information may be available at SHERPA/RoMEO