THE IMPORTANCE OF PHYSICAL MODELS FOR DERIVING DUST MASSES AND GRAIN SIZE DISTRIBUTIONS IN SUPERNOVA EJECTA. I. RADIATIVELY HEATED DUST IN THE CRAB NEBULA

Record Type

  • Journal Articles

Full Title

  • THE IMPORTANCE OF PHYSICAL MODELS FOR DERIVING DUST MASSES AND GRAIN SIZE DISTRIBUTIONS IN SUPERNOVA EJECTA. I. RADIATIVELY HEATED DUST IN THE CRAB NEBULA

Author(s)

  • Temim T, Dwek E

Publication Title

Publication Title (abbreviated)

  • ASTROPHYS J

Publication Date

  • 2013 Sep 1

DOI

  • 10.1088/0004-637X/774/1/8

ISSN

  • 0004-637X

Volume

  • 774

Issue

  • 1

Page Count

  • 8

Article Number

  • 8

Keyword(s)

Citation

  • Temim T, Dwek E. THE IMPORTANCE OF PHYSICAL MODELS FOR DERIVING DUST MASSES AND GRAIN SIZE DISTRIBUTIONS IN SUPERNOVA EJECTA. I. RADIATIVELY HEATED DUST IN THE CRAB NEBULA. ASTROPHYS J. 2013;774 (1):8.

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