Pulsating variable white dwarf (helium) stars and solitons

Details Pulsating variable white dwarf (helium) stars and solitons Pulsating variable white dwarf (helium) stars and solitons

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.179..155n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 179, no. 1, May 1991, p. 155-162.

Astronomy and Astrophysics

Astrophysics

Helium, Solitary Waves, Stellar Oscillations, Variable Stars, White Dwarf Stars, Light Curve, Stellar Spectra, Stellar Temperature

Scientific paper

The highly complex mode spectrum pattern of the May 28, 1982 emissions from the variable dwarf GD 358 reported by Winget et al. (1982) is interpreted in terms of soliton dispersions. It is suggested that the new approach provides a theoretical framework for understanding the chemistry of spatial stratification, excitation mechanisms, and the basic physics of white dwarfs.

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