Results 71 to 80 of about 1,219 (138)
KIC 3868420: A High-amplitude δ Scuti–γ Dor Hybrid Star Crossing the Hertzsprung Gap
We report a photometric and asteroseismic analysis of KIC 3868420, a newly identified high-amplitude δ Scuti– γ Doradus hybrid star located in the Hertzsprung gap—a short-lived and rarely observed post-main-sequence phase.
Tao-Zhi Yang, Zhao-Yu Zuo
doaj +1 more source
Variable stars in the globular cluster NGC 3201. I. Multimode SX Phe-type variables
We report on the discovery of eleven multimode SX Phoenicis--type blue stragglers in the field of the southern globular cluster NGC 3201. In these variables both radial and non-radial modes are excited.
Krzeminski, W. +2 more
core +1 more source
Hilbert Transform Reveals Unusual Modulation in Delta Scuti Star KIC 10407873
We report a δ Scuti star, KIC 10407873, exhibiting significant amplitude modulation. Fourier analysis of Kepler long-cadence data (i.e., Q0-Q17, spanning 1471 days) reveals two distinct features: harmonic series of frequencies in the low-frequency region
Haozhi Wang +5 more
doaj +1 more source
Modelling of the fast rotating delta Scuti star Altair
We present an asteroseismic study of the fast rotating star HD187642 (Altair), recently discovered to be a delta Scuti pulsator. We have computed models taking into account rotation for increasing rotational velocities.
Bruntt, H., Buzasi, D., Suarez, J. C.
core +1 more source
The Identification of RR Lyrae and Delta Scuti Stars from Variable GALEX Ultraviolet Sources
We identify the RR Lyrae and delta Scuti (DSCT) stars in three catalogs of GALEX variable sources. The NUV amplitude of RR Lyrae stars is about twice that in V-band, so we find a larger percentage of low amplitude variables than catalogs such as Abbas et al (2014).
Kinman, T. D., Brown, Warren R.
openaire +2 more sources
Signature of High-amplitude Pulsations in Seven δ Sct Stars via TESS Observations
The regular behavior of the pulsations of high-amplitude δ Sct (HADS) stars gives a greater chance to investigate the interiors of stars. We analyzed seven HADS stars showing peak-to-peak amplitudes of more than 0.3 mag that were newly observed by TESS ...
Fatemeh Vasigh +2 more
doaj +1 more source
Amplitude Variability in gamma Dor and delta Scuti stars observed by the Kepler Spacecraft
Proceedings of IAU Focus Meeting 17, Advances in Stellar Physics from Asteroseismology, XXIXth IAU General Assembly, Honolulu, Hawaii, August 2015. Focus meeting proceedings edited by C.S. Jeffery, J.A.
Guzik, Joyce A. +3 more
openaire +2 more sources
Analysis of pulsating variable stars using the visibility graph algorithm. [PDF]
Muñoz V, Garcés NE.
europepmc +1 more source
Asteroseismic modeling of high-amplitude δ Scuti (HADS) variables critically depends on their accurate classification, which provides robust constraints on stellar physical parameters.
Taozhi Yang, Zhaoyu Zuo
doaj +1 more source
We develop an ensemble machine learning framework to estimate key asteroseismic parameters—namely the frequency of the highest peak ( ν ( A _max )), the frequency of maximum oscillation power ( ν _max ), and the large frequency separation (Δ ν )—directly
Akram Bolouki +2 more
doaj +1 more source

