PG 0907+123 and JL 194: slowly pulsating hot subdwarf stars

Details PG 0907+123 and JL 194: slowly pulsating hot subdwarf stars PG 0907+123 and JL 194: slowly pulsating hot subdwarf stars

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010mnras.406.2701k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 406, Issue 4, pp. 2701-2712.

Astronomy and Astrophysics

Astronomy

1

Stars: Individual: Pg 0907+123, Stars: Individual: Jl 194, Stars: Oscillations, Subdwarfs, Stars: Variables: General

Scientific paper

Multicolour time-series photometry of two newly discovered slowly pulsating sdB stars (V1093 Her stars, also known as PG 1716 stars) is described. Both stars are fairly bright and appear, from the limited amount of data, to have rich pulsation spectra. Given that the amplitudes of variation of both stars are also large compared to most PG 1716 stars, both are good candidates for extensive follow-up observations.

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