Statistical Procedure for Computing Line-Blanketed Model Stellar Atmospheres.
نویسندگان
چکیده
منابع مشابه
Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation
Context. Very massive stars pass through the Wolf-Rayet (WR) stage before they finally explode. Details of their evolution have not yet been safely established, and their physics are not well understood. Their spectral analysis requires adequate model atmospheres, which have been developed step by step during the past decades and account in their recent version for line blanketing by the millio...
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ژورنال
عنوان ژورنال: The Astronomical Journal
سال: 1966
ISSN: 0004-6256
DOI: 10.1086/110142