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相关论文: Catalog of Galactic Beta Cephei Stars

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We present the results of a search for Galactic Beta Cephei stars, which are massive pulsating stars with both pressure modes and mixed modes. Thus, these stars can serve as benchmarks for seismological studies of the interiors of massive…

We analysed ASAS-3 photometry of bright early-type stars with the goal of finding new Beta Cephei stars. We were particularly interested in stars that would be good for seismic analysis, i.e., stars that (i) have a large number of excited…

天体物理学 · 物理学 2009-11-13 A. Pigulski , G. Pojmański

From the Fourier analysis of the catalogue of ~200,000 variable candidates in the OGLE-II Galactic fields, we found a sample of about 230 short-period low-amplitude variable stars. From their position in the colour-magnitude diagram and the…

天体物理学 · 物理学 2010-12-09 A. Narwid , Z. Kolaczkowski , A. Pigulski , T. Ramza

We present results of an analysis of the ASAS-3 data for short-period variables from the recently published catalogue of over 38 000 stars. Using the data available in the literature we verify the results of the automatic classification…

天体物理学 · 物理学 2007-05-23 A. Pigulski

This is a progress report of the study of pulsating main-sequence stars in the LMC. Using the OGLE-II photometry supplemented by the MACHO photometry, we find 64 Beta Cephei stars in the LMC. Their periods are generally much longer than…

The All Sky Automated Survey (ASAS) data, covering nearly 70% of the whole sky south of declination +28 deg, were recently used to discover about 300 Beta Cephei stars brighter than V~11.5 mag. As this means a nearly fourfold increase in…

太阳与恒星天体物理 · 物理学 2014-11-20 A. Pigulski , G. Pojmanski

Classification of over 50000 TESS stars in sectors 1-18 has resulted in the detection of 766 pulsating main sequence B stars as well as over 5000 $\delta$ Scuti, 2300 $\gamma$ Doradus and 114 roAp candidates. It is found that a distinct…

太阳与恒星天体物理 · 物理学 2020-03-18 Luis A Balona , Dogus Ozuyar

The combined strength of asteroseismology and empirical stellar basic parameter determinations for in-depth asteroseismic analysis of massive pulsators in eclipsing binaries shows great potential for treating the challenging and mysterious…

太阳与恒星天体物理 · 物理学 2024-03-20 Christian I. Eze , Gerald Handler

We present a systematic investigation of $\beta$ Cephei (BCEP) stars by integrating photometric data from the Transiting Exoplanet Survey Satellite (TESS) with astrometric parameters from Gaia Data Release 3. Utilizing TESS's short-cadence…

太阳与恒星天体物理 · 物理学 2025-12-16 Xiang-dong Shi , Sheng-bang Qian , Li-ying Zhu , Lin-jia Li , Er-gang Zhao , David Mkrtichian , Farkhodjon Khamrakulov , Wen-xu Lin

The Gaia mission detected many new candidate $\beta$ Cephei ($\beta$ Cep) pulsators, whose variability classification has since been confirmed from Transiting Exoplanet Survey Satellite (TESS) space photometry of the nominal mission. We aim…

太阳与恒星天体物理 · 物理学 2025-06-18 D. J. Fritzewski , M. Vanrespaille , C. Aerts , Z. Guo , D. Hey , J. De Ridder

$\beta$ Cephei pulsating variable (BCEP) stars are the most massive pulsating variable stars in the main sequence, exhibiting both p- and g-mode pulsations. In this study, we identified 155 BCEP stars or candidates using data from TESS and…

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 , Er-gang Zhao , Wen-xu Lin

The $\beta$ Cephei stars represent an important class of massive star pulsators probing the evolution of B-type stars and the transition from main sequence to hydrogen-shell burning evolution. By understanding $\beta$ Cep stars, we gain…

太阳与恒星天体物理 · 物理学 2015-12-02 Hilding R. Neilson , Richard Ignace

Studying stellar pulsations in open clusters offers the possibility to perform ensemble asteroseismology. The reasonable assumption that the cluster members have the same age, distance, and overall metallicity aids in the seismic modelling…

太阳与恒星天体物理 · 物理学 2015-05-28 G. Handler , S. Meingast

We present the results of a magnetic survey of a sample of eight beta Cephei stars and 26 Slowly Pulsating B stars with FORS1 at the VLT. A weak mean longitudinal magnetic field of the order of a few hundred Gauss is detected in the beta…

天体物理学 · 物理学 2009-11-11 S. Hubrig , M. Briquet , M. Schoeller , P. De Cat , G. Mathys , C. Aerts

We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small…

太阳与恒星天体物理 · 物理学 2009-11-13 S. Hubrig , M. Briquet , P. De Cat , M. Schoeller , T. Morel , I. Ilyin

We report a multisite photometric campaign for the Beta Cephei star 12 Lacertae. 750 hours of high-quality differential photoelectric Stromgren, Johnson and Geneva time-series photometry were obtained with 9 telescopes during 190 nights.…

The beta Cephei star delta Ceti was considered one of the few monoperiodic variables in the class. Despite (or perhaps because of) its apparently simple oscillation spectrum, it has been challenging and controversial to identify this star's…

We present preliminary results of multi-colour photometry of Beta Cephei stars observed in the LMC and in NGC 6200. Tentative identifications of pulsation modes have been made, and a number of new B pulsators have been noted. Interesting…

太阳与恒星天体物理 · 物理学 2012-06-29 C. Ulusoy , C. A. Engelbrecht , T. Gülmez

$\beta$ Cep stars in eclipsing binary (EB) systems give us an opportunity to put observational constraints on their structure and stellar parameters. We present a comprehensive analysis of the $\beta$ Cep star in the EB V446 Cep, using…

太阳与恒星天体物理 · 物理学 2026-05-08 A. Moharana , J. Southworth , K. Pavlovski , A. Miszuda , R. S. Rathour , K. G. Hełminiak , F. Marcadon , D. M. Bowman , T. B. Pawar , A. Tkachenko

We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowly Pulsating B stars. Roughly one third of the studied beta…

太阳与恒星天体物理 · 物理学 2009-01-22 S. Hubrig , M. Briquet , P. De Cat , M. Schoeller , T. Morel , I. Ilyin
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