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相关论文: On period distribution of RR Lyr type variables in…

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We obtained a series of more than two hundred R-band CCD images for the crowded central (115"x77") region of the metal-poor globular cluster M15 with an angular resolution of 0.5"-0.9" in most images. Optimal image subtraction was used to…

天体物理学 · 物理学 2009-11-10 Alexander P. Zheleznyak , Valery V. Kravtsov

The theory of stellar evolution can be more closely tested if we have the opportunity to measure new quantities. Nowadays, observations of galactic RR Lyr stars are available on a time baseline exceeding 100 years. Therefore, we can exploit…

天体物理学 · 物理学 2009-11-13 J. F. Le Borgne , A. Paschke , J. Vandenbroere , E. Poretti , A. Klotz , M. Boer , Y. Damerdji , M. Martignoni , F. Acerbi

We present theoretical predictions concerning horizontal branch stars in globular clusters, including RR Lyrae variables, as derived from synthetic procedures collating evolutionary and pulsational constraints. On this basis, we explore the…

天体物理学 · 物理学 2009-11-10 S. Cassisi , M. Castellani , F. Caputo , V. Castellani

We present the catalog of RR Lyrae stars discovered in a 4.5 square degrees area in the central parts of the Large Magellanic Cloud (LMC). Presented sample contains 7612 objects, including 5455 fundamental mode pulsators (RRab), 1655…

Evolution of Population I stars with initial masses from 70M_\odot to 130M_\odot is considered under various assumptions on the mass loss rate \dot M. The mass-luminosity relation of W-R stars is shown to be most sensitive to the mass loss…

天体物理学 · 物理学 2009-11-13 Yu. A. Fadeyev

We have performed a detailed study of the pulsational and evolutionary characteristics of 133 RR Lyrae stars in the globular cluster NGC5272 (M3) using highly accurate BVI data taken on 5 separate epochs. M3 seems to contain no less than…

天体物理学 · 物理学 2009-11-10 C. Cacciari , T. M. Corwin , B. W. Carney

The third part of the OGLE-III Catalog of Variable Stars comprises 24906 RR Lyr stars in the Large Magellanic Cloud (LMC). This sample consists of 17693 fundamental-mode (RRab), 4958 first-overtone (RRc), 986 double-mode (RRd) and 1269…

太阳与恒星天体物理 · 物理学 2009-04-03 I. Soszynski , A. Udalski , M. K. Szymanski , M. Kubiak , G. Pietrzynski , L. Wyrzykowski , O. Szewczyk , K. Ulaczyk , R. Poleski

We present new BV CCD photometry, light curves, and ephemerides for 9 previously known, 29 newly detected RR Lyrae variables and one newly detected variable of an unknown type in the globular cluster M75. The photometry used for the…

天体物理学 · 物理学 2009-11-07 T. M. Corwin , M. Catelan , H. A. Smith , J. Borissova , F. R. Ferraro , W. S. Raburn

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…

天体物理学 · 物理学 2009-11-10 M. Castellani , F. Caputo , V. Castellani

Globular clusters offer a powerful way to test the properties of stellar populations and the late stages of low-mass stellar evolution. In this paper we study oscillating giant stars and overtone RR Lyrae-type pulsators in the nearest…

太阳与恒星天体物理 · 物理学 2025-10-15 László Molnár , Henryka Netzel , Madeline Howell , Csilla Kalup , Meridith Joyce

We present the results of a photometric study of RR Lyrae variables in the field of the globular cluster M55. We have discovered nine new RR Lyrae stars, increasing the number of known variables in this cluster to 15 objects. Five of the…

天体物理学 · 物理学 2009-10-31 A. Olech , J. Kaluzny , I. B. Thompson , W. Pych , W. Krzeminski , A. Schwarzenberg-Czerny

The ninth part of the OGLE-III Catalog of Variable Stars (OIII-CVS) comprises RR Lyr stars in the Small Magellanic Cloud (SMC). Our sample consists of 2475 variable stars, of which 1933 pulsate in the fundamental mode (RRab), 175 are the…

太阳与恒星天体物理 · 物理学 2010-09-29 I. Soszynski , A. Udalski , M. K. Szymanski , M. Kubiak , G. Pietrzynski , L. Wyrzykowski , K. Ulaczyk , R. Poleski

Evolutionary sequences of AGB stars with initial masses on the main sequence $M_\mathrm{ZAMS}=1.5M_\odot$, $2M_\odot$ and $3M_\odot$ were computed for the initial metallicity $Z=0.014$. Selected models of evolutionary sequences with…

太阳与恒星天体物理 · 物理学 2023-12-14 Yu. A. Fadeyev

We report the results of CCD V and R photometry of the RR Lyrae stars in M2. The periodicities of most variables are revised and new ephemerides are calculated. Light curve decomposition of the RR Lyrae stars was carried out and the…

天体物理学 · 物理学 2009-11-11 C. Lazaro , A. Arellano Ferro , M. J. Arevalo , D. M. Bramich , S. Giridhar , E. Poretti

Secular period variations, $\beta=\dot{P}$, in 76 RR Lyrae stars in the globular cluster M5 are analysed using our most recent CCD $V$ photometry and the historical photometric database available in the literature since 1889. This provides…

太阳与恒星天体物理 · 物理学 2016-06-15 A. Arellano Ferro , J. A. Ahumada , N. Kains , A. Luna

We present the results of a time-resolved photometric and time-series analysis of a RR Lyrae type star RR Gem. The main results are as follows: We found RR Gem's pulsation period, 0.39689 d, and its V and I mean magnitudes, 11.277 (V) and…

太阳与恒星天体物理 · 物理学 2019-08-30 V. A. Gohil , S. P. Bhatnagar

We present the first simultaneous photometric and spectroscopic investigation of a large set of RR Lyrae variables in a globular cluster. The radial-velocity data presented comprise the largest sample of RVs of RR Lyrae stars ever obtained.…

We present a comprehensive catalog of 2824 RR Lyrae stars (RRLs) residing in 115 Galactic globular clusters (GCs). Our catalog includes 1594 fundamental-mode (RRab), 824 first-overtone (RRc), and 28 double-mode (RRd) RRLs, as well as 378…

太阳与恒星天体物理 · 物理学 2024-02-15 Mauricio Cruz Reyes , Richard I. Anderson , Lucas Johansson , Henryka Netzel , Zoé Medaric

Stellar evolution calculations were carried out from the main sequence to the final AGB stage of stars with initial masses from 1 to $2M_\odot$ and metallicity $Z=0.01$. Selected models of evolutionary sequences were used as initial…

太阳与恒星天体物理 · 物理学 2018-09-11 Yuri Fadeyev

New BVI CCD photometry is presented for 60 RR Lyrae variables in the globular cluster M3. Light curves have been constructed and ephemerides have been (re)-derived for all of them. Four stars (i.e. V29, V136, V155 and V209), although…

天体物理学 · 物理学 2009-10-30 E. Carretta , C. Cacciari , F. R. Ferraro , F. Fusi Pecci , G. Tessicini