Results 1 to 10 of about 12,020 (316)
γ Doradus Stars: Defining a New Class of Pulsating Variables [PDF]
15 pages, 1 ps figure.
Anthony B Kaye +2 more
exaly +5 more sources
A Catalog of New Slowly Pulsating B-type Stars
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
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
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
Pulsating stars in NGC 6231 Frequency analysis and photometric mode identification near the main sequence [PDF]
We used Johnson UBV photometric CCD observations to identify pulsating and other variable stars in the young open cluster NGC 6231. The multi-color information was used to classify pulsating variables, perform frequency analysis, and - where possible ...
Handler, Gerald +2 more
core +1 more source
Discovery of magnetic fields in three He variable Bp stars with He and Si spots [PDF]
It is essential for the understanding of stellar structure models of high mass stars to explain why constant stars, non-pulsating chemically peculiar hot Bp stars and pulsating stars co-exist in the slowly pulsating B stars and beta Cephei instability ...
Aerts +20 more
core +2 more sources
The impact of large-scale, long-term optical surveys on pulsating star research
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
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 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
A unifying explanation of complex frequency spectra of gamma Dor, SPB and Be stars: combination frequencies and highly non-sinusoidal light curves [PDF]
There are many Slowly Pulsating B (SPB) stars and γ Dor stars in the Kepler mission data set. The light curves of these pulsating stars have been classified phenomenologically into stars with symmetric light curves and with asymmetric light curves.
Bedding, T. R. +4 more
core +3 more sources

