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Balloon 090100001: A bright, high amplitude sdB pulsator

TLDR
In this paper, the authors reported the discovery of pulsations in the light curve of Balloon 090100001, a bright sdB star from the balloon-borne survey of Bixler et al.
Abstract
We report the discovery of pulsations in the light curve of Balloon 090100001, a bright sdB star () from the balloon-borne survey of Bixler et al. (1991). Our time series observations made with the IAC80 telescope reveal a powerful short period oscillation with a period of 356 s and an amplitude (~59 mmag) only matched in all of the sdB pulsators by the main pulsation of PG 1605+072. The first harmonic (at 178 s) and another independent period (at 264 s) are also present in the amplitude spectrum of this new EC 14026 star. New spectroscopic data from the William Herschel Telescope provide the parameters K and dex. These place Balloon 090100001 in the low temperature and low gravity corner of the sdBV instability region, making it an interesting target for study of possible frequency changes due to stellar evolution.

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Journal ArticleDOI

HS 0702+6043: a star showing both short-period p-mode and long-period g-mode oscillations

TL;DR: In this paper, the photometric variability of the hot subdwarf B star HS 0702+6043 was analyzed and interpreted in order to explore its asteroseismological potential.
Journal ArticleDOI

A survey for pulsating subdwarf B stars with the Nordic Optical Telescope

TL;DR: In this article, a search for pulsating subdwarf B stars was conducted with the Nordic Optical Telescope on La Palma over 59 nights between 1999 and 2009, and twenty new short period pulsators were found.
Journal ArticleDOI

A survey for pulsating subdwarf B stars with the Nordic Optical Telescope

TL;DR: In this article, a search for pulsating subdwarf B stars was conducted with the Nordic Optical Telescope on La Palma over 59 nights between 1999 and 2009, and twenty new pulsators were found, most of which have already been published and some extensively studied.
References
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Journal ArticleDOI

The origin of subdwarf B stars – I. The formation channels

TL;DR: In this paper, a detailed investigation of the three main binary evolution channels that can lead to the formation of sdB stars: the common-envelope (CE) ejection channel, the stable Roche lobe overflow (RLOF) channel, and the double helium white dwarfs (WDs) merger channel is presented.
Journal ArticleDOI

The Origin of Subdwarf B Star (I): the Formation Channels

TL;DR: In this article, the authors investigated the three main binary evolution channels that can lead to the formation of sdB stars: the common envelope (CE) ejection channel, the stable Roche lobe overflow (RLOF) channel and the double helium white dwarfs (WDs) merger channel.
Journal ArticleDOI

A spectroscopic determination of the mass distribution of DA white dwarfs

TL;DR: In this paper, a mass distribution for a sample of 129 DA white dwarfs is presented, based on fitting hydrogen line profiles to the predictions of stellar atmosphere models, and the atmospheric parameters determined from spectroscopy are shown to be of improved accuracy over those obtained with other techniques.
Journal ArticleDOI

Ultraviolet Radiation from Evolved Stellar Populations. I. Models

TL;DR: In this article, an extensive grid of calculations of stellar models from the zero-age horizontal branch (ZAHB) through to a point late in post-HB evolution or a point on the white dwarf cooling track is presented.
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