Nova Vulpeculae 1984-2 near the maximum of light

Details Nova Vulpeculae 1984-2 near the maximum of light Nova Vulpeculae 1984-2 near the maximum of light

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..187a&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 187-191 (SEE N86-20287 10-93)

Other

5

Light Curve, Novae, Stellar Spectra, Stellar Spectrophotometry, Line Spectra, Magnesium, Stellar Cores, Stellar Mass Accretion, White Dwarf Stars

Scientific paper

The spectra of Nova Vul 1984-2 are discussed. They are like the spectra of other novae near maximum of light, but Nova Vul 1984-2 is a typical slow nova. The most unusual spectroscopic feature of this nova seems to be the relative strength of Mg II and Mg I lines. As turbulent mixing between the white dwarf and the accreted material can lead to CNO enrichments, such a mixing of core matter can explain the overabundance of Mg if one assumes a massive O-Ne-Mg white dwarf.

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