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相关论文: A survey for pulsating subdwarf B stars with the N…

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We report the results of our search for pulsating subdwarf B stars in Full Frame Images, sampled at 30 min cadence and collected during Year 1 of the TESS mission. Year 1 covers most of the southern ecliptic hemisphere. The sample of…

太阳与恒星天体物理 · 物理学 2020-11-09 S. K. Sahoo , A. S. Baran , S. Sanjayan , J. Ostrowski

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 used to separate the objects into accurate classes, and we…

We report the results of our search for pulsating subdwarf B stars in Full Frame Images collected during Year 2 of the TESS mission and covering the northern ecliptic hemisphere. This is a continuation of our effort we presented in Paper I.…

太阳与恒星天体物理 · 物理学 2021-05-05 A. S. Baran , S. K. Sahoo , S. Sanjayan , J. Ostrowski

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 continuous month-long Kepler datasets of these 5 objects; these…

We search for new variable B-type pulsators in the CoRoT data assembled primarily for planet detection, as part of CoRoT's Additional Programme. We aim to explore the properties of newly discovered B-type pulsators from the uninterrupted…

We present results from the first two quarters of a survey to search for pulsations in compact stellar objects with the Kepler spacecraft. The survey sample and the various methods applied in its compilation are described, and spectroscopic…

We continue our program of single-site observations of pulsating subdwarf B (sdB) stars and present the results of extensive time series photometry of HS 0039+4302 and HS 0444+0458. Both were observed at MDM Observatory during the fall of…

天体物理学 · 物理学 2009-06-23 M. D. Reed , D. M. Terndrup , A. -Y. Zhou , C. T. Unterborn , D. An , J. R. Eggen

We present results of a continuation of our Transiting Exoplanet Survey Satellite (TESS) search for short-period pulsations in compact stellar objects observed during Years 2 and 4 of the TESS mission that targeted the northern ecliptic…

太阳与恒星天体物理 · 物理学 2024-03-06 A. S. Baran , S. Charpinet , R. H. Østensen , M. D. Reed , V. Van Grootel , C. Lyu , J. H. Telting , P. Németh

We present results of a Transiting Exoplanet Survey Satellite (TESS) search for short-period pulsations in compact stellar objects observed in years 1 and 3 of the TESS mission, during which the southern ecliptic hemisphere was targeted. We…

太阳与恒星天体物理 · 物理学 2023-01-11 A. S. Baran , V. Van Grootel , R. H. Ostensen , H. L. Worters , S. K. Sahoo , S. Sanjayan , S. Charpinet , P. Nemeth , J. H. Telting , D. Kilkenny

This paper reports the discovery of new slowly pulsating B-type stars. Based on the photometric, spectral, and astrometric data of TESS, LAMOST, and Gaia surveys, we have found 286 new slowly pulsating B-type stars (SPB stars) and 21…

太阳与恒星天体物理 · 物理学 2024-12-06 Xiang-dong Shi , Sheng-bang Qian , Li-ying Zhu , Lin-jia Li

Hot subdwarf B (sdB) stars are post-main-sequence stars of high temperature and gravity. Approximately 30$\%$ of sdBs exhibit stable pressure and/or gravity-mode pulsations, which can be used via the timing method to test for companion…

太阳与恒星天体物理 · 物理学 2025-08-05 Tomomi Otani , A. S. Baran , Lindsay C. Spence , Ted von Hippel , E. Lynum-Lozano , Julia. M. Clark

We report the discovery of four new pulsating subdwarf B (sdBV) stars from Campaign 7 of the Kepler spacecraft's K2 mission. EPICs 215776487, 217280630, 218366972, and 218717602 are all gravity (g)-mode pulsators and we also detect two…

太阳与恒星天体物理 · 物理学 2021-09-01 M. D. Reed , A. J. Slayton , A. S. Baran , J. H. Telting , R. H. Ostensen , C. S. Jeffery , M. Uzundag , S. Sanjayan

Hot subdwarf B (sdB) stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant stars lose their hydrogen envelope via interactions with close companions. They play an important role in our understanding of…

We collected a sample of ten hitherto unidentified SPB stars with the aim of describing their pulsational properties and identifying pulsational modes. Photometric time series data from various surveys were collected and analyzed using…

太阳与恒星天体物理 · 物理学 2020-01-22 M. Fedurco , E. Paunzen , S. Hümmerich , K. Bernhard , Š. Parimucha

The survey phase of the Kepler Mission includes a number of hot subdwarf B (sdB) stars to search for nonradial pulsations. We present our analysis of two sdB stars that are found to be g-mode pulsators of the V1093 Her class. These two…

The 60 known rapidly oscillating Ap (roAp) stars are excellent laboratories to test pulsation models in the presence of stellar magnetic fields. Our survey is dedicated to search for new group members in the Northern Hemisphere. We attempt…

太阳与恒星天体物理 · 物理学 2015-06-23 E. Paunzen , M. Netopil , M. Rode-Paunzen , G. Handler , H. Bozic

A search was carried out for pulsars with periods (P) from 2 to 90 s in daily observations carried out over an interval of 5 years in a area measuring 6300 sq.deg. The data was obtained on a Large Phased Array (LPA) at a frequency of 111…

高能天体物理现象 · 物理学 2025-04-22 S. A. Tyul'bashev , G. E. Tyul'basheva

In 2007, a companion with planetary mass was found around the pulsating subdwarf B star V391 Pegasi with the timing method, indicating that a previously undiscovered population of substellar companions to apparently single subdwarf B stars…

We report results of our analysis of the Kepler superaperture LC data of the open cluster NGC6791 to search for pulsating sdB stars. We checked all pixels and we found only three sdB stars to be pulsating, KIC2569576 (B3), KIC2438324 (B4)…

太阳与恒星天体物理 · 物理学 2021-11-19 S. Sanjayan , A. S. Baran , J. Ostrowski , P. Németh , I. Pelisoli , R. Østensen , J. W. Kern , M. D. Reed , S. K. Sahoo

We present the results of a survey using the WASP archive to search for high frequency pulsations in F-, A- and B-type stars. Over 1.5 million targets have been searched for pulsations with amplitudes greater than 0.5 millimagnitude. We…

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