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The evolution of circumstellar matter around an isolated massive star during the red supergiant phase - the role of heat conduction
Author(s) -
A. D’Ercole
Publication year - 1992
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1093/mnras/255.4.572
Subject(s) - physics , astrophysics , nebula , supergiant , supernova , thermal conduction , radius , astronomy , red supergiant , stellar evolution , star (game theory) , phase (matter) , stars , computer security , computer science , quantum mechanics , thermodynamics

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