The first view of δ Scuti and γ Doradus stars with the TESS mission
We present the first asteroseismic results for δ Scuti and γ Doradus stars observed in
Sectors 1 and 2 of the TESS mission. We utilize the 2-min cadence TESS data for a sample …
Sectors 1 and 2 of the TESS mission. We utilize the 2-min cadence TESS data for a sample …
Measuring mean densities of δ Scuti stars with asteroseismology-theoretical properties of large separations using TOUCAN
Aims. We study the theoretical properties of the regular spacings found in the oscillation
spectra of δ Scuti stars. Methods. We performed a multivariable analysis that covered a wide …
spectra of δ Scuti stars. Methods. We performed a multivariable analysis that covered a wide …
Asteroseismology of a Double-mode High-amplitude δ Scuti Star TIC 448892817
C Lv, A Esamdin, J Pascual-Granado… - The Astronomical …, 2022 - iopscience.iop.org
We propose that TIC 448892817 is a double-mode high-amplitude δ Scuti star. The radial
modes detected in this star provide a unique opportunity to exploit asteroseismic techniques …
modes detected in this star provide a unique opportunity to exploit asteroseismic techniques …
Variable stars in the Fornax dSph Galaxy. II. Pulsating stars below the horizontal branch
E Poretti, G Clementini, EV Held, C Greco… - The Astrophysical …, 2008 - iopscience.iop.org
We have carried out an intensive survey of the northern region of the Fornax dwarf
spheroidal galaxy with the aim of detecting the galaxy's short-period pulsating stars (P< 0.25 …
spheroidal galaxy with the aim of detecting the galaxy's short-period pulsating stars (P< 0.25 …
The OGLE Collection of Variable Stars. Over 15,000 Delta Scuti Stars in the Large Magellanic Cloud
I Soszyński, P Pietrukowicz, A Udalski… - arXiv preprint arXiv …, 2023 - arxiv.org
We present the OGLE collection of delta Scuti stars in the Large Magellanic Cloud and in its
foreground. Our dataset encompasses a total of 15,256 objects, constituting the largest …
foreground. Our dataset encompasses a total of 15,256 objects, constituting the largest …
Kepler observations of the high-amplitude δ Scuti star V2367 Cyg
LA Balona, P Lenz, V Antoci, S Bernabei… - Monthly Notices of …, 2012 - academic.oup.com
We analyse Kepler observations of the high-amplitude δ Scuti (HADS) star V2367 Cyg (KIC
9408694). The variations are dominated by a mode with frequency f 1= 5.6611 d− 1. Two …
9408694). The variations are dominated by a mode with frequency f 1= 5.6611 d− 1. Two …
Exploring the variable stars in the globular cluster NGC 5024 (M53): new RR Lyrae and SX Phoenicis stars
A Arellano Ferro, R Figuera Jaimes… - Monthly Notices of …, 2011 - academic.oup.com
We report CCD V and I time series photometry of the globular cluster NGC 5024 (M53). The
technique of difference image analysis has been used which enables photometric …
technique of difference image analysis has been used which enables photometric …
TIC 308396022: δ Scuti–γ Doradus hybrid with large-amplitude radial fundamental mode and regular g-mode period spacing
TZ Yang, ZY Zuo, G Li, TR Bedding, SJ Murphy… - Astronomy & …, 2021 - aanda.org
We analyse the pulsating behaviour of TIC 308396022, based on observations by the TESS
mission. The star is a high-amplitude δ Sct star that shows a very rich amplitude spectrum …
mission. The star is a high-amplitude δ Sct star that shows a very rich amplitude spectrum …
A New Census of the Variable Star Population in the Globular Cluster NGC 2419
M Di Criscienzo, C Greco, V Ripepi… - The Astronomical …, 2011 - iopscience.iop.org
We present B, V, and I CCD light curves for 101 variable stars belonging to the globular
cluster NGC 2419, 60 of which are new discoveries, based on data sets obtained at the …
cluster NGC 2419, 60 of which are new discoveries, based on data sets obtained at the …
Precise Evolutionary Asteroseismology of High-Amplitude δ Scuti Star AE Ursae Majoris
HF Xue, JS Niu, JN Fu - Research in Astronomy and Astrophysics, 2022 - iopscience.iop.org
Stellar structure and evolution theory is one of the bases in modern astronomy. Stellar inner
structures and their evolutionary states can be precisely tested by asteroseismology, since …
structures and their evolutionary states can be precisely tested by asteroseismology, since …