Results 21 to 30 of about 501 (275)

A Catalog of New Slowly Pulsating B-type Stars

open access: yesThe Astrophysical Journal Supplement Series, 2023
This paper reports the discovery of new slowly pulsating B-type stars. Based on the photometric, spectral, and astrometric data of the TESS, LAMOST, and Gaia surveys, we have found 286 new slowly pulsating B-type (SPB) stars and 21 candidates.
Xiang-dong Shi   +3 more
doaj   +1 more source

Magnetic Activity of Different Types of Variable Stars Observed by TESS Mission

open access: yesUniverse, 2023
The investigation of the magnetic activity of different types of variable stars holds significant implications for our understanding of the physical processes and evolution of stars.
Ming Zhong   +3 more
doaj   +1 more source

Magnetic and pulsational variability of Przybylski’s star (HD 101065) [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
11 pages, 4 tables, 7 figures, accepted for publication in ...
Hubrig, S.   +6 more
openaire   +2 more sources

The pulsating variable star population in DDO210 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
We have probed the pulsating variable star content of the isolated Local Group dwarf galaxy, DDO210 (Aquarius), using archival Advanced Camera for Surveys/$Hubble$ $Space$ $Telescope$ imaging in the F475W and F814W passbands. We find a total of 32 RR Lyrae stars (24 ab-type, 8 c-type) and 75 Cepheid variables. The mean periods of the ab-type and c-type
Ordoñez, Antonio J., Sarajedini, Ata
openaire   +2 more sources

FX UMa: A New Heartbeat Binary System with Linear and Nonlinear Tidal Oscillations and δ Sct Pulsations

open access: yesThe Astronomical Journal, 2023
We present a detailed analysis of an eclipsing double-lined binary FX UMa based on TESS photometry and newly acquired spectroscopic observations. The radial velocities and atmospheric parameters for each component star are obtained from the SONG high ...
Kun Wang   +5 more
doaj   +1 more source

Variability and pulsations in the Be star 66 Ophiuchi [PDF]

open access: yesAstronomy & Astrophysics, 2002
Oph is a Be star seen under a moderate inclination angle that shows strong variability from UV to IR wavelengths. A concise review of long-term variability history is given. High resolution, high S /N spectroscopic observations obtained in 1997, 1998 and 2001 and spectropolarimetric observations obtained in 2000 are presented.
Floquet, M.   +11 more
openaire   +4 more sources

Pulsating star research and the Gaia revolution

open access: yesEPJ Web of Conferences, 2017
In this article we present an overview of the ESA Gaia mission and of the unprecedented impact that Gaia will have on the field of variable star research.
Eyer Laurent   +19 more
doaj   +1 more source

The impact of large-scale, long-term optical surveys on pulsating star research

open access: yesEPJ Web of Conferences, 2017
The era of large-scale photometric variability surveys began a quarter of a century ago, when three microlensing projects - EROS, MACHO, and OGLE - started their operation.
Soszyński Igor
doaj   +1 more source

Multifilter Time-series Observations of Eleven Blue Short-period ATLAS Variable Stars

open access: yesThe Astronomical Journal, 2023
Eleven periodic variable stars were observed photometrically through two to four filters from the set UBVR _C I _C . Phase-folded data for each star cover full cycles of variation.
C. Koen, V. Schaffenroth, A. Kniazev
doaj   +1 more source

Eclipsing Systems with Pulsating Components (Types β Cep, δ Sct, γ Dor or Red Giant) in the Era of High-Accuracy Space Data

open access: yesGalaxies, 2021
Eclipsing systems are essential objects for understanding the properties of stars and stellar systems. Eclipsing systems with pulsating components are furthermore advantageous because they provide accurate constraints on the component properties, as well
Patricia Lampens
doaj   +1 more source

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