Results 11 to 20 of about 2,822 (109)

Variable Stars in Local Group Galaxies. IV. RR Lyrae stars in the central regions of the low-density galaxy Crater II [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
We present a search and analysis of variable stars in the recently discovered Crater~II dwarf galaxy. Based on $B$, $V$, $I$ data collected with the Isaac Newton Telescope (FoV$\sim$0.44 square degrees) we detected 37 variable stars, of which 34 are bone-
Andreuzzi, G.   +11 more
core   +6 more sources

A Catalogue of RR Lyrae Stars from the Northern Sky Variability Survey

open access: yesMonthly Notices of the Royal Astronomical Society, 2006
A search for RR Lyrae stars has been conducted in the publicly available data of the Northern Sky Variability Survey (NSVS). Candidates have been selected by the statistical properties of their variation; the standard deviation, skewness and kurtosis ...
Akerlof   +41 more
core   +3 more sources

Multiperiodic Galactic field RR Lyrae stars in the ASAS catalog [PDF]

open access: yes, 2007
The All Sky Automated Survey (ASAS) monitors bright stars (8 mag < V < 14 mag) south of declination +28 deg. The ASAS Catalogue of Variable Stars (ACVS) presently contains 50,099 objects; among them are 2212 objects classified as RR Lyrae pulsating ...
Fabrycky, D. C., Szczygiel, D. M.
core   +4 more sources

A Study of Double- and Multi-mode RR Lyrae Variables

open access: yesOpen Astronomy, 2015
We present the results of our new study of known RR Lyrae variable stars. All observations available for these stars in the Catalina Surveys were analyzed, and double-mode variations were identified.
Khruslov A. V.
doaj   +1 more source

The EPOCH Project: I. Periodic variable stars in the EROS-2 LMC database [PDF]

open access: yes, 2014
The EPOCH (EROS-2 periodic variable star classification using machine learning) project aims to detect periodic variable stars in the EROS-2 light curve database. In this paper, we present the first result of the classification of periodic variable stars
Bailer-Jones, Coryn A. L.   +6 more
core   +1 more source

The QUEST RR Lyrae Survey: III. The Low Galactic Latitude Catalogue [PDF]

open access: yes, 2012
We present results for the QUEST RR Lyrae Survey at low galactic latitude, conducted entirely with observations obtained with the QUEST mosaic camera and the 1.0/1.5m J\"urgen Stock Schmidt telescope at the National Observatory of Venezuela.
Briceño, César   +5 more
core   +2 more sources

Gaia Data Release 2: Validation of the classification of RR Lyrae and Cepheid variables with the Kepler and K2 missions [PDF]

open access: yes, 1912
The second data release of the Gaia mission includes an advance catalog of variable stars. The classification of these stars are based on sparse photometry from the first 22 months of the mission.
Molnár, László   +3 more
core   +2 more sources

Newly Discovered RR Lyrae Stars in the SDSSXPanXSTARRS1XCatalina Footprint [PDF]

open access: yes, 2014
We present the detection of 6,371 RR Lyrae (RRL) stars distributed across ~14,000 deg^2 of the sky from the combined data of the Sloan Digital Sky Survey (SDSS), the Panoramic Survey Telescope and Rapid Response System 1 (PS1), and the second photometric
Abbas, M. A.   +5 more
core   +1 more source

Pulsating Variable Stars in the Coma Berenices dwarf spheroidal galaxy

open access: yes, 2009
We present B, V, I time-series photometry of the Coma Berenices dwarf spheroidal galaxy, a faint Milky Way satellite, recently discovered by the Sloan Digital Sky Survey.
Belokurov   +47 more
core   +1 more source

Fourier decomposition and frequency analysis of the pulsating stars with P < 1day in the OGLE database. II. Multiperiodic RR Lyrae variables in the Galactic Bulge [PDF]

open access: yes, 2002
We present the results of a systematic search for multiperiodic pulsators among the Galactic Bulge RR Lyrae stars of the OGLE-1 sample. We identify one "canonical" double-mode variable (RRd star) pulsating in two radial modes.
Alcock   +18 more
core   +2 more sources

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