Amplitude and frequency variability of the pulsating DB white dwarf stars KUV 05134+2605 and PG 1654+160 observed with the Whole Earth Telescope
Open Access
- 11 April 2003
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 340 (3) , 1031-1038
- https://doi.org/10.1046/j.1365-8711.2003.06373.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 20 references indexed in Scilit:
- The asteroseismological potential of the pulsating DB white dwarf stars CBS 114 and PG 1456+103Monthly Notices of the Royal Astronomical Society, 2002
- Discovery and asteroseismological analysis of a new pulsating DB white dwarf star, PG 2246+121Monthly Notices of the Royal Astronomical Society, 2001
- Delta Scuti Network observations of XX Pyx: detection of 22 pulsation modes and of short-term amplitude and frequency variationsMonthly Notices of the Royal Astronomical Society, 2000
- On the frequency and amplitude variations of the Scuti star CD-24 7599 (=XX Pyx)Monthly Notices of the Royal Astronomical Society, 1998
- New Whole Earth Telescope observations of CD-24 7599: steps towards Scuti star seismologyMonthly Notices of the Royal Astronomical Society, 1997
- Asteroseismological Observations of the Central Star of the Planetary Nebula NGC 1501The Astronomical Journal, 1996
- The WET Standard PhotometerPublications of the Astronomical Society of the Pacific, 1996
- The potential for asteroseismology of DB white dwarf starsThe Astrophysical Journal, 1993
- High-precision time-resolved CCD photometryPublications of the Astronomical Society of the Pacific, 1992
- KUV 05134 + 2605 - A new pulsating DB white dwarfThe Astronomical Journal, 1989