Break-up of quasi-periodic motion as an interpretation of white-dwarf variability

Details Break-up of quasi-periodic motion as an interpretation of white-dwarf variability Break-up of quasi-periodic motion as an interpretation of white-dwarf variability

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.188..137d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 188, no. 1, Feb. 1992, p. 137-142.

Astronomy and Astrophysics

Astrophysics

1

Poincare Problem, Power Spectra, Stellar Oscillations, Stellar Spectrophotometry, White Dwarf Stars, Coupled Modes, Light Curve, Variable Stars

Scientific paper

High-speed photometric data obtained for a number of white-dwarf stars
confirm the presence of subharmonic frequency in their power spectra. As
many of these white dwarfs show multiperiodic structures, we show that
the break up of quasi-periodic motion results in the appearance of
similar subharmonic components in their spectra

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