White Dwarf Observations in Hungary

Details White Dwarf Observations in Hungary White Dwarf Observations in Hungary

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..334..597p&link_type=abstract

14th European Workshop on White Dwarfs, ASP Conference Series, Vol. 334 Proceedings of a meeting held at Kiel, July 19-23, 2004

Astronomy and Astrophysics

Astronomy

Scientific paper

The Hungarian contribution on the white dwarfs PG 1654+160 and KPD 1930+2752 (WET targets Xcov 21 and Xcov 23) is presented by a team from the Konkoly Observatory. The short time-scale amplitude and frequency variability of PG 1654+160 is based on our single site observations. The amplitude variation of the dominant pulsational mode of KPD 1930+2752 over a month is demonstrated. At two nights (20/21 Aug and 6/7 Sep 2003) there were no modes excited above the noise level. Based on 8 nights single site observation only 7 frequencies were derived from the 44 excited modes published previously.

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