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Related papers: Exploring M33 Through RR Lyrae Stars

200 papers

We present an overview of our study of the short period variable stars in the Large Magellanic Cloud, and in the dwarf galaxies Fornax, Leo I, and NGC 6822. Light curves are presented for RR Lyrae stars, Anomalous Cepheids and, for the…

Astrophysics · Physics 2007-05-23 G. Clementini

That the RR Lyrae star period -- K-band luminosity relation is a promising tool as a distance indicator in the Milky Way and Local Group of Galaxies is apparent on observational and theoretical grounds in the literature. Less clear is the…

Astrophysics · Physics 2009-11-07 D. J. Butler

Low-mass, variable, high-velocity stars are interesting study cases for many aspects of Galactic structure and evolution. Until recently, the only known high- or hyper-velocity stars were young stars thought to originate from the Galactic…

Solar and Stellar Astrophysics · Physics 2016-05-04 Camilla Juul Hansen , Robert Michael Rich , Andreas Koch , Siyi Xu , Andrea Kunder , Hans-Guenter Ludwig

RR Lyrae variables are excellent population II distance indicators thanks to their well-defined period-luminosity relations (PLRs) at infrared wavelengths. We present results of near-infrared (NIR) monitoring of Galactic globular clusters…

We have measured radial velocities and metallicities of 16 RR Lyrae stars, from the QUEST survey, in the Sagittarius tidal stream at 50 kpc from the galactic center. The distribution of velocities is quite narrow (std dev=25 km/s)…

Astrophysics · Physics 2007-05-23 A. Katherina Vivas , Robert Zinn , Carme Gallart

The Milky Way (MW) stellar halo, containing debris from past accretion events, serves as a fossil record of hierarchical mass assembly. Due to their distinct properties, RR Lyrae stars (RRLs) serve as excellent tracers for identifying and…

Astrophysics of Galaxies · Physics 2026-04-29 T. Muraveva , L. Monti , D. Massari , M. De Leo , A. Garofalo , G. Clementini , E. Ceccarelli , U. Michelucci

[ABRIDGED] $\omega$ Centauri (NGC 5139) contains large numbers of variable stars of different types and, in particular, more than a hundred RR Lyrae stars. We have conducted a variability survey of $\omega$ Cen in the NIR, using ESO's 4.1m…

Solar and Stellar Astrophysics · Physics 2015-05-13 C. Navarrete , R. Contreras Ramos , M. Catelan , C. M. Clement , F. Gran , J. Alonso-García , R. Angeloni , M. Hempel , I. Dékány , D. Minniti

We present an analysis of the relative abundance features of a number of chemical elements in the atmospheres of metal-rich ($\rm{[Fe/H]} > -1.0$) Galactic-field RR~Lyrae variable stars and the kinematic characteristics of these stars. We…

Solar and Stellar Astrophysics · Physics 2024-08-07 M. L. Gozha , V. A. Marsakov , V. V. Koval'

We analyze the kinematics and spatial distribution of 15,599 fundamental-mode RR Lyrae (RRL) stars in the Milky Way bulge by combining OGLE-IV photometric data and Gaia DR2 proper motions. We show that the longitudinal proper motions and…

Astrophysics of Galaxies · Physics 2020-10-14 Hangci Du , Shude Mao , E. Athanassoula , Juntai Shen , Pawel Pietrukowicz

Observational bias against finding Milky Way (MW) dwarf galaxies at low Galactic latitudes (b < 20 deg) and at low surface brightnesses (fainter than 29 mag arcsec^-2, in the V-band) currently limits our understanding of the faintest limits…

Astrophysics of Galaxies · Physics 2015-11-11 Mariah Baker , Beth Willman

We present a kinematical study of 314 RR~Lyrae stars in the solar neighbourhood using the publicly available photometric, spectroscopic, and {\it Gaia} DR2 astrometric data to explore their distribution in the Milky Way. We report an…

Solar and Stellar Astrophysics · Physics 2020-04-21 Z. Prudil , I. Dékány , E. K. Grebel , A. Kunder

We present the results of a search for short-period variable stars in Leo A. We have found 92 candidate variables, including eight candidate RR Lyrae stars. From the RR Lyraes, we measure a distance modulus of (m-M)_0 = 24.51 +/- 0.12, or…

We report on new B, V and I CCD photometry of the globular cluster M54 that was aimed at the study of its variable stars. With respect to the previous most recent work on M54 we have nearly doubled the number of detected variable stars: M54…

Astrophysics · Physics 2007-05-23 Carla Cacciari , Michele Bellazzini , Samantha Colucci

We report the spectroscopic analysis of 20 halo ab-type RR Lyrae stars with heliocentric distances between 15 and 165 kpc, conducted using medium-resolution spectra from the Magellan Inamori Kyocera Echelle (MIKE) spectrograph. We obtain…

We have undertaken a search for variable stars in the metal-rich globular cluster NGC 6441 using time-series BV photometry. The total number of variables found near NGC 6441 has been increased to ~104, with 48 new variables being found in…

Astrophysics · Physics 2009-11-06 Barton J. Pritzl , Horace A. Smith , Marcio Catelan , Allen V. Sweigart

The spectacular data delivered by NASA's {\it Kepler} mission have not only boosted the discovery of planets orbiting other stars, but they have opened a window on the inner workings of the stars themselves. For the study of the RR Lyrae…

Solar and Stellar Astrophysics · Physics 2013-10-03 Katrien Kolenberg

Results of a search for variable stars in the central region of the globular cluster M13 are presented. Prior to this study, 36 variable and suspected variable stars were known in this cluster (Osborn 2000; Clement et al. 2001). Of these…

Astrophysics · Physics 2009-11-07 G. Kopacki , Z. Kolaczkowski , A. Pigulski

We report the discovery of an intriguing triple-mode RR Lyrae star found in the OGLE Galactic bulge collection, OGLE-BLG-RRLYR-24137. In the OGLE catalog the star was identified as RRd star - double-mode pulsator, pulsating simultaneously…

We discuss the first part of a survey for RR Lyrae variables in the galactic halo that is being made with the 1m Schmidt telescope at the Venezuelan National Observatory. So far the survey has discovered 497 variables in 380 sq. degrees,…

Astrophysics · Physics 2007-05-23 A. Katherina Vivas , Robert Zinn

The metal content of the spiral galaxy M33 is analyzed through spectroscopic observations of its emission-line populations, H ii regions and Planetary Nebulae (PNe): their abundance gradients are identical within the errors. The 2D…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-10 Laura Magrini