Stability and Radial Vibration Periods of the Hamada-Salpeter White Dwarf Models

Details Stability and Radial Vibration Periods of the Hamada-Salpeter White Dwarf Models Stability and Radial Vibration Periods of the Hamada-Salpeter White Dwarf Models

May 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968natur.218..734f&link_type=abstract

Nature, Volume 218, Issue 5143, pp. 734-736 (1968).

Physics

34

Scientific paper

The rapidly pulsating radio sources may, after all, be vibrating white
dwarfs. Calculations show that fundamental vibration periods for white
dwarfs can be as low as ~1.5 s.

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