Results 111 to 120 of about 5,541 (198)
Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-variable Horizontal-branch Stars. III. M55 and NGC 6362 [PDF]
Don A. VandenBerg, Pavel A. Denissenkov
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Classification of Periodic Variable Stars from TESS
The number of known periodic variable stars has increased rapidly in recent years. As an all-sky transit survey, the Transiting Exoplanet Survey Satellite (TESS) plays an important role in detecting low-amplitude variable stars.
Xinyi Gao +3 more
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The ancient stellar population of M 32: RR Lyrae variable stars confirmed [PDF]
G. Fiorentino +4 more
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Multiband light curves of two RR Lyrae variables in Segue II and Ursa Major II ultrafaint dwarf galaxies were collected from near simultaneous observations using the Lulin One-meter Telescope in Vgri bands.
Chow-Choong Ngeow, Anupam Bhardwaj
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Stellar Atmospheric Parameters of ∼11,000 RR Lyrae Stars from LAMOST Spectra
Accurate determination of the stellar atmospheric parameters of RR Lyrae stars (RRLs) requires short individual exposures of the spectra to mitigate pulsation effects.
Jiangtao Wang +4 more
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Color–Magnitude Diagram of NGC 205 and Its RR Lyrae Variables
We present the deepest color–magnitude diagram (CMD) for NGC 205 in the F606W (≈ V ) and F814W (≈ I ) filters. Our archival Hubble Space Telescope/Advanced Camera for Surveys field is centered ∼3 $\mathop{.}\limits^{{\rm{^{\prime} }}}$ 8 northwest of the
Ata Sarajedini
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Period Changes of Mira Variables, RR Lyrae Stars, and Type II Cepheids [PDF]
H. A. Smith
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The Lack of RR Lyrae Variables in Ultrafaint Dwarf Galaxy Sextans II
RR Lyrae in ultrafaint dwarf (UFD) galaxies, if found, would be valuable to constrain the distances of these UFD. In this work, we report our search of RR Lyrae in a recently discovered UFD—Sextans II. Based on multiband (griz) time-series archival DECam
Chow-Choong Ngeow, Anupam Bhardwaj
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Variable stars in the Gaia era: Mira, RR Lyrae, δ and Type-II Cepheids [PDF]
Martin A. T. Groenewegen
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First Detection of Shock Waves in RRc Stars
Although shock waves have been well documented in fundamental-mode RRab stars, their existence in first-overtone pulsator stars, RRc stars, has remained uncertain. Building upon the spectroscopic frameworks established by M. Chadid et al., we present the
Junzhang Li, Merieme Chadid
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