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相关论文: The Absolute Magnitude of RRc Variables From Stati…

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We present a mathematical analysis of the statistical parallax method. The method yields physical insight into the maximum-likelihood determinations of the luminosity and velocity distribution and enables us to conduct a vigorous Monte…

天体物理学 · 物理学 2008-02-03 Piotr Popowski , Andrew Gould

We present new statistical parallax solutions for the absolute magnitude and kinematics of RR Lyrae stars. New proper motion, radial velocity, and abundance data are used; the new data set is 50% larger, and of higher quality, than…

天体物理学 · 物理学 2009-10-28 A. C. Layden , R. B. Hanson , S. L. Hawley , A. R. Klemola , C. J. Hanley

The present determination of the absolute magnitude $M_V(RR)$ of RR Lyrae stars is twofold, relying upon Hipparcos proper motions and trigonometric parallaxes separately. First, applying the statistical parallax method to the proper…

天体物理学 · 物理学 2014-10-13 Takuji Tsujimoto , Masanori Miyamoto , Yuzuru Yoshii

We use UCAC4 proper motions and WISE W1-band apparent magnitudes intensity-mean for almost 400 field RR Lyrae variables to determine the parameters of the velocity distribution of Galactic RR Lyrae population and constrain the zero points…

星系天体物理 · 物理学 2013-09-19 A. K. Dambis , L. N. Berdnikov , A. Y. Kniazev , V. V. Kravtsov , A. S. Rastorguev , R. Sefako , O. V. Vozyakova

All galaxies that have been adequately examined so far have shown an extended stellar halo. To search for such a halo in the LMC we have obtained low-resolution spectra for 100 LMC RR Lyrae stars, of which 87 are in the field and 13 in the…

天体物理学 · 物理学 2009-11-11 J. Borissova , D. Minniti , M. Rejkuba , D. Alves

We present a catalog of 5,290 RR Lyrae stars (RRLs) with metallicities estimated from spectra of the LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) and the Sloan Extension for Galactic Understanding and Exploration…

太阳与恒星天体物理 · 物理学 2020-04-15 G. -C. Liu , Y. Huang , H. -W. Zhang , M. -S. Xiang , J. -J. , Ren , B. -Q. Chen , H. -B. Yuan , C. Wang , Y. Yang , Z. -J. Tian , F. Wang , X. -W. Liu

In this paper we investigate whether a misestimate of proper motions could have been a source of substantial systematic errors in the statistical parallax determination of the absolute magnitude of RR Lyrae stars. In an earlier paper, we…

天体物理学 · 物理学 2007-05-23 Piotr Popowski , Andrew Gould

I review statistical parallax absolute magnitude determinations which employ data from the HIPPARCOS satellite for RR Lyrae and Cepheid variables, and for several other stellar classes. Five groups have studied the RR Lyrae stars, and the…

天体物理学 · 物理学 2007-05-23 Andrew C. Layden

We present the radial velocities, metallicities and the K-band magnitudes of 74 RR Lyrae stars in the inner regions of the LMC. The intermediate resolution spectra and infrared images were obtained with FORS1 at the ESO VLT and with the…

天体物理学 · 物理学 2009-11-10 J. Borissova , D. Minniti , M. Rejkuba , D. Alves , K. H. Cook , K. C. Freeman

We present new absolute trigonometric parallaxes and proper motions for seven Pop II variable stars: five RR Lyr variables; RZ Cep, XZ Cyg, SU Dra, RR Lyr, UV Oct; and two type 2 Cepheids; VY Pyx and {\kappa} Pav. We obtained these results…

Full space velocities are computed for a sample of 130 nearby RR Lyrae variables using both ground-based and Hipparcos proper motions. In many cases proper motions from multiple sources have been averaged to produce a significant…

天体物理学 · 物理学 2009-10-30 John C. Martin , Heather L. Morrison

We present new time-series CCD \emph{VR} photometry of the globular cluster NGC 5634. We aim to use the known RR Lyrae stars, members of the cluster, as indicators of mean metallicity and distance. Accurate coordinates, periods and an…

太阳与恒星天体物理 · 物理学 2025-07-21 A. Arellano Ferro , R. Michel , M. A. Yepez , S. Muneer , I. Bustos Fierro , Z. Prudil

We present V-band CCD photometry of 65 RR Lyr variables from the globular cluster M5. We have estimated the basic physical parameters for 16 RRc stars and 26 RRab stars using a Fourier decomposition of the light curves of the variables. The…

天体物理学 · 物理学 2007-05-23 J. Kaluzny , A. Olech , I. Thompson , W. Pych , W. Krzeminski , A. Schwarzenberg-Czerny

We have calculated the physical parameters of the RR Lyrae stars in the globular cluster NGC~4147 via the Fourier decomposition of their light curves, using new data and well-established semi-empirical calibrations and zero points. The mean…

太阳与恒星天体物理 · 物理学 2018-03-15 A. Arellano Ferro , F. C. Rojas Galindo , S. Muneer , Sunetra Giridhar

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

太阳与恒星天体物理 · 物理学 2023-02-22 Xin-Yi Li , Yang Huang , Gao-Chao Liu , Timothy C. Beers , Hua-Wei Zhang

We present a careful and detailed light curve analysis of publicly available $I$-band data on fundamental mode RR Lyrae (RRab) stars of the Large Magellanic Cloud (LMC) obtained by the Optical Gravitational Lensing Experiment (OGLE)…

太阳与恒星天体物理 · 物理学 2015-06-18 Sukanta Deb , Harinder P. Singh

This paper presents results from photometric and statistical-parallax analysis of a sample of 850 field RR Lyrae (RRL) variables. The photometric and spectroscopic data for sample RRLs are obtained from (1) our new spectroscopic…

星系天体物理 · 物理学 2021-02-10 T. D. Muhie , A. K. Dambis , L. N. Berdnikov , A. Y. Kniazev , Eva K. Grebel

In this paper, we report the detections of stellar variabilities from the first 2-year observations of sky area of about 1300 square degrees from the Tsinghua University-NAOC Transient Survey (TNTS). A total of 1237 variable stars…

太阳与恒星天体物理 · 物理学 2015-09-23 Xinyu Yao , Lingzhi Wang , Xiaofeng Wang , Tianmeng Zhang , Juncheng Chen , Wenlong Yuan , Jun Mo , Wenxiong Li , Zhiping Jin , Xuefeng Wu , JunDan Nie , Xu Zhou
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