Results 41 to 50 of about 2,888,460 (154)

Abundance analysis of seven delta Scuti stars

open access: yes, 2008
Context: The current knowledge of the abundance pattern in delta Scuti stars is based on analysis of just a few field stars. Aims: We aim to determine the general chemical properties of the atmospheres of delta Scuti stars based on a statistically ...
Fossati, L.   +7 more
core   +1 more source

Observations and a new interpretation for the Delta Scuti variable star VZ CANCRI

open access: yesThe Astrophysical Journal, 1984
Extensive numbers of new photoelectric data have been collected and analyzed to investigate the modal behavior of VZ Cnc. Its previously observed periods yield a period ratio of 0.80 implying pulsation in the first and second radial overtones. Of the seventeen delta Scuti stars listed by Fitch and Sziedl which have well-determined periods, it is the ...
A. N. Cox, B. J. McNamara, W. Ryan
openaire   +1 more source

Asteroseismic Determination of Stellar Rotation: On Synchronization in the Close Eclipsing Binaries AB Cas and OO Dra

open access: yesThe Astrophysical Journal, 2023
A star’s rotation rate is difficult to estimate without surface inhomogeneities such as dark or bright spots. This paper presents asteroseismic results to determine the rotation rates of δ Sct-type pulsating primary stars in two eclipsing binary systems,
Seung-Lee Kim
doaj   +1 more source

A grid of 200 000 models of young δ Scuti stars using mesa and GYRE [PDF]

open access: yes, 2023
The rapidly increasing number of delta Scuti stars with regular patterns among their pulsation frequencies necessitates modelling tools to better understand the observations.
Bedding, Timothy R.   +3 more
core   +1 more source

The study of short orbital period delta Scuti pulsating variable star

open access: yes, 2019
In this contribution, we pointed out the applicability of Modified binarogram in detecting low orbit Kepler binaries.
Yasin Abduselam Mohammed, Feleke Getinet
openaire   +3 more sources

Solar-like oscillations in Delta Scuti stars [PDF]

open access: yes, 2011
Diese Dissertation befasst sich mit der Suche nach sonnenähnlichen Oszillationen in Delta Scuti Sternen. Theoretische Modelle deuten darauf hin, dass die Konvektion in den äußeren Schichten dieser Sterne noch effektiv genug ist, um diese Art Pulsationen
Antoci, Victoria Laura
core  

The pulsation of Delta Scuti stars [PDF]

open access: yes, 2014
A theoretical study of the pulsation of Delta Scuti stars is presented. A modified Henyey code is used to produce a grid of evolutionary models of population I composition, spanning the area of the Instability Strip on and near the Main Sequence ...
Milligan, Helen
core   +2 more sources

Oscillation frequencies of moderately rotating delta scuti stars: asymmetric mode splittings due to non-spherical distortion [PDF]

open access: yes
We find that the observed pressure-mode rotational splittings of slowly/moderately rotating Scuti stars and Cephei stars mostly have a positive asymmetry.
Kurtz, Donald W.   +11 more
core   +1 more source

Determination of oscillation frequencies and stellar properties of three Delta Scuti variable stars using Kepler data

open access: yesJournal of the National Science Foundation of Sri Lanka, 2020
Asteroseismology is the science that deals with the oscillations in the stars with the goal of understanding the stellar structure. In this study, photometric data of Kepler mission have been used for the asteroseismic study of Delta Scuti type pulsating stars. The light curve analysis of three Delta Scuti stars observed by Kepler mission is presented.
J. Adassuriya   +3 more
openaire   +2 more sources

A magnetic study of the δ Scuti variable HD 21190 and the close solar-type background star CPD −83°64B [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
HD 21190 is a known $\delta$ Scuti star showing Ap star characteristics and a variability period of 3.6 h discovered by the Hipparcos mission. Using Gaia DR1 data for an astrometric analysis, it was recently suggested that HD 21190 forms a physical binary system with the companion CPD -83$^{\circ}$ 64B.
S P Järvinen   +5 more
openaire   +2 more sources

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