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Author Gaur, V. P. ♦ Tripathi, B. M. ♦ Joshi, G. C. ♦ Pande, M. C.
Source Aryabhatta Research Institute of Observational Sciences (ARIES)
Content type Text
File Format PDF
Language English
Subject Domain (in DDC) Natural sciences & mathematics ♦ Physics
Subject Keyword DA White dwarfs
Abstract Molecular dissociation equilibrium calculations were done for the model atmospheres of DA and non-DA white dwarfs. Our calculations show that He₂⁺ and HeH⁺ appears as most abundant molecules in the atmospheres of non-DA white dwarfs while H₂and He₂⁺ are most abundant molecules in DA white dwarfs. It is suggested that these molecules should be searched for in the atmospheres of white dwarfs.
Part of series ass147-107
Educational Use Research
Education Level UG and PG
Learning Resource Type Article