collaborators

9 papers

astro-ph.SR2011

GALEX J201337.6+092801: The lowest gravity subdwarf B pulsator

Roy H Østensen, Peter I Pápics, Raquel Oreiro +8

We present the recent discovery of a new subdwarf B variable (sdBV), with an exceptionally low surface gravity. Our spectroscopy of J20136+0928 places it at Teff = 32100 +/- 500, l…

astro-ph.SR2011

First Kepler results on compact pulsators VII. Pulsating subdwarf B stars detected in the second half of the survey phase

A. S. Baran, S. D. Kawaler, M. D. Reed +10

We present five new pulsating subdwarf B (sdB) stars discovered by the Kepler spacecraft during the asteroseismology survey phase. We perform time-series analysis on the nearly con…

astro-ph.SR2011

First Kepler results on compact pulsators VIII: Mode identifications via period spacings in mode pulsating Subdwarf B stars

M. D. Reed, A. Baran, A. C. Quint +13

We investigate the possibility of nearly-equally spaced periods in 13 hot subdwarf B (sdB) stars observed with the Kepler spacecraft and one observed with CoRoT. Asymptotic limits…

astro-ph.SR2011

First Kepler results on compact pulsators VI. Targets in the final half of the survey phase

R. H. Østensen, R. Silvotti, S. Charpinet +29

We present results from the final six months of a survey to search for pulsations in white dwarfs and hot subdwarf stars with the Kepler spacecraft. Spectroscopic observations are…

astro-ph.SR2010

Whole Earth Telescope Observations of the subdwarf B star KPD 1930+2752: A rich, short period pulsator in a close binary

M. D. Reed, S. L. Harms, S. Poindexter +58

KPD 1930+2752 is a short-period pulsating subdwarf B (sdB) star. It is also an ellipsoidal variable with a known binary period just over two hours. The companion is most likely a w…

astro-ph.SR2010

First Kepler results on compact pulsators II: KIC 010139564, a new pulsating subdwarf B (V361 Hya) star with an additional low-frequency mode

Steven D. Kawaler, M. D. Reed, A. C. Quint +13

We present the discovery of nonradial pulsations in a hot subdwarf B star based on 30.5 days of nearly continuous time-series photometry using the \emph{Kepler} spacecraft. KIC 010…