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Related papers: SALT and RR Lyrae variables: Our Galaxy, The Magel…

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We discuss recent developments on the age and metallicity distribution for early type galaxies in different environments.

Astrophysics · Physics 2008-11-07 Duncan A. Forbes , Alejandro I. Terlevich

We summarize past and current surveys for Wolf-Rayet stars among the Local Group galaxies, emphasizing both the how and the why. Such studies are invaluable for helping us learn about massive star evolution, and for providing sensitive…

Solar and Stellar Astrophysics · Physics 2015-08-03 Philip Massey , Kathryn F. Neugent , Nidia Morrell

We compute the spatial velocity components and the galactic orbital elements for 209 metal-poor $([Fe/H] < -1.0)$ RRLyrae (ab) variable stars in the solar neighborhood using proper motions, radial velocities, and photometric distances…

Astrophysics · Physics 2009-11-07 T. V. Borkova , V. A. Marsakov

The serendipitous discovery by Preston and colleagues of the neutron-capture-enhanced RR Lyrae variable star TY Gru (a.k.a. CS 22881-071 in the "HK" survey of very metal-poor halo stars) has resulted in a growing set of initiatives on the…

Solar and Stellar Astrophysics · Physics 2011-08-26 Christopher Sneden , Bi-Qing For , George W. Preston

Dwarf galaxies in the local group provide a unique astrophysical laboratory. Despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history.…

Astrophysics · Physics 2007-05-23 Jan Snigula , Claus Goessl , Ulrich Hopp , Heinz Barwig

We employ a sample of 135,873 RR Lyrae stars (RRLs) with precise photometric-metallicity and distance estimates from the newly calibrated $P$--$\phi_{31}$--$R_{21}$--[Fe/H] and $Gaia$ $G$-band $P$--$R_{21}$--[Fe/H] absolute…

We are carrying out a comprehensive multi-wavelength study of dwarf galaxies in the Local Volume (< 5 Mpc). After our all-sky survey more than doubled the dwarf census we are now measuring structural parameters, integrated properties, and…

Measurements of [Fe/H] and radial velocity are presented for 89 RR Lyrae (RRL) candidates within 6 kpc of the Sun. After removal of two suspected non-RRL, these stars were added to an existing database, which yielded 464 RRL with [Fe/H] on…

Astrophysics of Galaxies · Physics 2020-01-08 R. Zinn , X. Chen , A. C. Layden , D. I. Casetti-Dinescu

An introduction is given to projects investigating galaxy evolution quantitatively by spectroscopic observations of very distant galaxies that have weak apparent brightnesses and small sizes as it is feasible with 10m-class telescopes like…

Astrophysics · Physics 2007-05-23 Bodo L. Ziegler

With ages comparable to the age of the Universe, the variable stars of RR Lyrae type have eyewitnessed the formation of their host galaxies, and thus can provide information on the processes that led to the assembling of large galaxies such…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-09 Gisella Clementini

The VMC survey is obtaining multi-epoch photometry in the Ks band of the Magellanic System down to a limiting magnitude of Ks ~ 19.3 for individual epoch data. The observations are spaced in time such as to provide optimal sampling of the…

This is the third in a series of papers studying the variable stars in old globular clusters in the Large Magellanic Cloud. The primary goal of this series is to look at how the characteristics and behavior of RR Lyrae stars in…

Local galaxies follow scaling relations between mass and stellar population properties such as age and metallicity, which encode key information on their evolutionary histories. We revise these relations using the largest spectroscopic…

Astrophysics of Galaxies · Physics 2025-11-05 D. Mattolini , S. Zibetti , A. R. Gallazzi , L. Scholz-Diaz , J. Pratesi

The Vista Magellanic Cloud (VMC, PI M.R. Cioni) survey is collecting $K_S$-band time series photometry of the system formed by the two Magellanic Clouds (MC) and the "bridge" that connects them. These data are used to build $K_S$-band light…

Solar and Stellar Astrophysics · Physics 2015-06-04 V. Ripepi , M. I. Moretti , G. Clementini , M. Marconi , M. R. Cioni , J. B. Marquette , P. Tisserand

We argue that, at least a fraction of the newly discovered population of ultra-faint dwarf spheroidal galaxies in the Local Group constitute the fossil relic of a once ubiquitous population of dwarf galaxies formed before reionization with…

Astrophysics · Physics 2011-02-11 Mia S. Bovill , Massimo Ricotti

We review the formation and evolution of fossil groups and clusters from both the theoretical and the observational points of view. In the optical band, these systems are dominated by the light of the central galaxy. They were interpreted…

Cosmology and Nongalactic Astrophysics · Physics 2021-06-28 J. Alfonso L. Aguerri , Stefano Zarattini

In this paper we revisit observational data concerning RR Lyrae stars in Galactic globular clusters, presenting frequency histograms of fundamentalized periods for the 32 clusters having more than 12 pulsators with well recognized period…

Astrophysics · Physics 2009-11-10 M. Castellani , F. Caputo , V. Castellani

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

RR Lyrae are a well-known class of pulsating horizontal branch stars widely used as tracers of old, metal-poor stellar populations. However, mounting observational evidence shows that a significant fraction of these stars may be young and…

Solar and Stellar Astrophysics · Physics 2024-01-17 Alexey Bobrick , Giuliano Iorio , Vasily Belokurov , Joris Vos , Maja Vuckovic , Nicola Giacobbo

I discuss Local Group galaxies from the perspective of external galaxies that define benchmark scaling relations. Making use of this information leads to a model for the Milky Way that includes bumps and wiggles due to spiral arms. This…

Astrophysics of Galaxies · Physics 2023-05-02 Stacy McGaugh
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