Results 111 to 120 of about 1,219 (138)
Abstract Gaia DR3 revealed 748,058 pulsating variable stars of mixed DSCT∣GDOR∣SXPHE types. This project undertakes a comprehensive examination to validate and distinguish these stars using Transiting Exoplanet Survey Satellite data. Aiming for reliable catalogs of bona fide δ Scuti and γ Doradus stars, I have validated 1715 δ Scuti ...
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The structure of the Milky Way from period-luminosity relations. [PDF]
Skowron DM.
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An Investigation of Short-Period Variable Stars. I. The Delta Scuti Stars
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Pulsational mode-typing in line profile variables. IV - Selected Delta Scuti stars
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Short-period variability of B, A and F stars. II. Photometry of new delta Scuti stars.
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Publications of the Astronomical Society of the Pacific, 1990
The observational history of the Delta Scuti star AI CVn wasa traced, and it was found to be incomplete and contradictory. It is suggested that the star is misclassified as a spectroscopic binary in The Bright Star Catalogue and that simultaneous spectroscopic and photometric observations are needed to determine the true nature of this star.
Jeremy R. King, Tianxing Liu
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The observational history of the Delta Scuti star AI CVn wasa traced, and it was found to be incomplete and contradictory. It is suggested that the star is misclassified as a spectroscopic binary in The Bright Star Catalogue and that simultaneous spectroscopic and photometric observations are needed to determine the true nature of this star.
Jeremy R. King, Tianxing Liu
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The study of short orbital period of delta scuti pulsating variable stars
Proceedings of the International Astronomical Union, 2019AbstractAs a pulsating star moves in its binary orbit, the path length of the light between us and the star varies, leading to the periodic variation in the arrival time of the signal from the star to us (earth). With the consideration of pulsators light arrival time delay effects several new methods which allows using Kepler photometric data (light ...
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Rapidly oscillating Ap stars and Delta Scuti variables
2008The discovery of the rapidly oscillating Ap stars has raised many questions concerning the relationship among 6 Sct variables, Ap stars, and other apparent non-varying stars in the 6 Set instability strip. In this paper, the present status of our under standing of the rapidly oscillating Ap stars and the δ Set stars is reviewed, but the former class is
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2021
Сообщается об обнаружении 44 новых переменных звезд типа Дельта Щита высокой амплитуды с двойной периодичностью, тип HADS(B), пульсирующих в основном тоне и в первом обертоне. Проанализированы все имеющиеся для этих звезд наблюдения из открытого онлайн-архива ASAS-SN с использованием программного обеспечения для поиска периодов, разработанного В.П ...
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Сообщается об обнаружении 44 новых переменных звезд типа Дельта Щита высокой амплитуды с двойной периодичностью, тип HADS(B), пульсирующих в основном тоне и в первом обертоне. Проанализированы все имеющиеся для этих звезд наблюдения из открытого онлайн-архива ASAS-SN с использованием программного обеспечения для поиска периодов, разработанного В.П ...
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Study of the variability of the Delta Scuti-stars
Astrophysics and Space Science, 1982Michele Bossi +3 more
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