Results 21 to 30 of about 36,168 (295)

Periodic variable A-F spectral type stars in the northern TESS continuous viewing zone. I. Identification and classification [PDF]

open access: yesAstronomy & Astrophysics, 2022
The goal of our study is to provide a reliable classification of variability of A-F stars brighter than 11 mag located in the northern TESS continuous viewing zone. We also aim at thorough discussion about issues in the classification related to the data
M. Skarka   +13 more
semanticscholar   +1 more source

Investigating Stellar Variability in the Open Cluster Region NGC 381

open access: yesThe Astronomical Journal, 2023
We study variable stars in the field of the open cluster NGC 381 using photometric data observed over 27 nights and identify a total of 57 variable stars, six of which are member stars. The variable stars are classified based on their periods, amplitudes,
Jayanand Maurya   +3 more
doaj   +1 more source

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

Highlights of Discoveries for δ Scuti Variable Stars From the Kepler Era [PDF]

open access: yesFrontiers in Astronomy and Space Sciences, 2021
The NASA Kepler and follow-on K2 mission (2009–2018) left a legacy of data and discoveries, finding thousands of exoplanets, and also obtaining high-precision long time-series data for hundreds of thousands of stars, including many types of pulsating ...
J. Guzik
semanticscholar   +1 more source

Variable Stars in the Giant Satellite Galaxy Antlia 2 [PDF]

open access: yesAstrophysical Journal, 2021
We report 350 pulsating variable stars found in four DECam fields (∼12 deg2) covering the Antlia 2 satellite galaxy. The sample of variables includes 318 RR Lyrae stars and eight anomalous Cepheids in the galaxy.
A. K. Vivas   +5 more
semanticscholar   +1 more source

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

The Secret Lives of Cepheids: δ Cep—The Prototype of a New Class of Pulsating X-Ray Variable Stars [PDF]

open access: yes, 2017
From our Secret Lives of Cepheids program, the prototype Classical Cepheid, δ Cep, is found to be an X-ray source with periodic pulsation-modulated X-ray variations.
S. Engle   +6 more
semanticscholar   +1 more source

Asteroseismic analysis of variable hot subdwarf stars observed with TESS [PDF]

open access: yesAstronomy & Astrophysics, 2021
Context. We present photometric and spectroscopic analyses of gravity (g-mode) long-period pulsating hot subdwarf B (sdB) stars, also called V1093 Her stars, observed by the TESS space telescope in both 120 s short-cadence and 20 s ultra-short-cadence ...
M. Uzundag   +10 more
semanticscholar   +1 more source

Pulsating stars in NGC 6231 Frequency analysis and photometric mode identification near the main sequence [PDF]

open access: yes, 2013
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

A search for variable subdwarf B stars in TESS Full Frame Images – II. Variable objects in the northern ecliptic hemisphere [PDF]

open access: yes, 2021
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.
A. Baran   +3 more
semanticscholar   +1 more source

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