KUV 05134 + 2605 - A new pulsating DB white dwarf

Details KUV 05134 + 2605 - A new pulsating DB white dwarf KUV 05134 + 2605 - A new pulsating DB white dwarf

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....98.2221g&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 98, Dec. 1989, p. 2221-2224.

Astronomy and Astrophysics

Astronomy

12

Stellar Oscillations, Stellar Spectrophotometry, White Dwarf Stars, Light Curve, Power Spectra, Pulsars, Spectral Energy Distribution, Stellar Evolution, Stellar Interiors, Stellar Temperature

Scientific paper

Time-series photometry is reported that shows that KUV 05134 + 2605 is a pulsating DB white dwarf. The light curve shows sharply peaked pulses with a complicated mode structure including periods between 350 and 900 sec. The optical spectrum appears to be that of a star near the hot end of the DB sequence, consistent with theoretical predictions and the temperature range estimated empirically for previously known DBV stars.

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