Results 101 to 110 of about 363 (172)
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
doaj +1 more source
The Evolutionary Status of M3 RR Lyrae Variable Stars: Breakdown of the Canonical Framework?
8 figures, 11 pages. Uses latest emulateapj.cls style file (included, 05/14/03) and apjfonts.sty (also included). The full-resolution preprint can be downloaded from http://www.astro.puc.cl/~mcatelan/.
openaire +5 more sources
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
doaj +1 more source
Variable stars in the Gaia era: Mira, RR Lyrae, δ and Type-II Cepheids [PDF]
Martin A. T. Groenewegen
openalex +1 more source
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
doaj +1 more source
Data smashing: uncovering lurking order in data. [PDF]
Chattopadhyay I, Lipson H.
europepmc +1 more source
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
doaj +1 more source
RR Lyrae Stars in Galactic Globular Clusters. II. A Theoretical Approach to Variables in M3 [PDF]
M. Marconi +3 more
openalex +1 more source
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
doaj +1 more source

