Consequences of a chromospheric temperature rise on the formation of the H line in late-type supergiants
Author(s) -
Sushma V. Mallik,
D. C. V. Mallik
Publication year - 1988
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/233.3.649
Subject(s) - physics , astrophysics , chromosphere , stars , supergiant , line (geometry) , radiative transfer , ionization , late type star , astronomy , spectral line , stellar atmosphere , optics , ion , geometry , mathematics , quantum mechanics
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