Results 101 to 110 of about 1,219 (138)
We present homogeneous, near-infrared ( JHK _s bands) time-series observations of the classical Carina dwarf spheroidal (dSph) galaxy to determine accurate and precise distances using the pulsating stars as standard candles.
Chow-Choong Ngeow +3 more
doaj +1 more source
A study of pulsation & rotation in a sample of A-K type stars in the Kepler field. [PDF]
Chowdhury S +5 more
europepmc +1 more source
δ Scuti variables are found at the intersection of the classical instability strip and the main sequence on the Hertzsprung–Russell diagram. With space-based photometry providing millions of light curves of A-F type stars, we can now probe the occurrence
Keyan Gootkin +5 more
doaj +1 more source
Citation-based clustering of publications using CitNetExplorer and VOSviewer. [PDF]
van Eck NJ, Waltman L.
europepmc +1 more source
A Note on the Variation of Delta Scuti. [PDF]
Sterne TE.
europepmc +1 more source
Establishing Baselines for Six Short-period δ Scuti Variables
As part of our variable star follow-up program, we have examined a number of stars from the Asteroid Terrestrial-impact Last Alert System (ATLAS) survey. Using a combination of our own data, ATLAS data, and other archival data, we confirmed the published
Christiana Z. Suggs +2 more
doaj +1 more source
The Transiting Exoplanet Survey Satellite (TESS) mission measured light from stars in ∼85% of the sky throughout its 2 yr primary mission, resulting in millions of TESS 30-minute-cadence light curves to analyze in the search for transiting exoplanets. To
Greg Olmschenk +11 more
doaj +1 more source
A Search of Periodic Variable Stars in the LMC by JWST Photometry
Based on high-resolution near-infrared photometric data from the James Webb Space Telescope (JWST) targeting the Large Magellanic Cloud, this study attempts to evaluate the feasibility and sensitivity limits of variable star detection in crowded stellar ...
Jiyu Wang +5 more
doaj +1 more source
Stability and Dynamics of Three-mode Coupling in δ Scuti Stars
Recent observations of δ Scuti stars find evidence of nonlinear three-mode coupling in their oscillation spectra. There are two types of three-mode coupling likely to be important in δ Scuti stars: (i) direct coupling, in which two linearly unstable ...
Mohammed Mourabit, Nevin N. Weinberg
doaj +1 more source
δ Scuti variables are found at the intersection of the classical instability strip and the main sequence on the Hertzsprung-Russell diagram. With space-based photometry providing millions of light-curves of A-F type stars, we can now probe the occurrence rate of δ Scuti pulsations in detail.
Gootkin, Keyan +5 more
openaire +2 more sources

