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相关论文: Probing the galactic halo with RR Lyrae stars I: T…

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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 present our analysis of a large sample (over 150k) of candidate Galactic RR Lyrae (RRL) stars for which we derived high quality photometry at UV, optical and infrared wavelengths, using data from publicly available surveys. For a…

Hypervelocity stars (HVSs) are stars with velocities exceeding their local escape velocities. Searching for HVSs and studying their origins can be an important way to study the properties of the Milky Way. In this paper, we utilize precise…

星系天体物理 · 物理学 2025-10-01 Haozhu Fu , Yang Huang , Huawei Zhang

Most of known RR Lyraes are type ab RR Lyraes (RRLab), and they are the excellent tool to map the Milky Way and its substructures. We find that 1148 RRLab stars determined by Drake et al.(2013) have been observed by spectroscopic surveys of…

星系天体物理 · 物理学 2018-03-28 Iminhaji Ablimit , Gang Zhao

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

RR Lyrae stars are excellent tracers of stellar populations for old, metal-poor components in the Milky Way Galaxy and the Local Group. Their luminosities have a metallicity-dependence, but determining spectroscopic [Fe/H] metallicities for…

Accurate determination of the stellar atmospheric parameters of RR Lyrae stars (RRLs) requires short individual exposures of the spectra to mitigate pulsation effects. We present improved template matching methods to determine the stellar…

太阳与恒星天体物理 · 物理学 2024-04-25 Jiangtao Wang , Jianrong Shi , Jianning Fu , Weikai Zong , Chunqian Li

We present a catalogue of 551,214 main-sequence stars in the local ($d < 2$ kpc) Galactic thick disk and halo, based on a search of stars with large proper motions ($\mu_{\mathrm{tot}} > 40.0$ mas/yr) in the Gaia Early Data Release 3. We…

星系天体物理 · 物理学 2022-01-05 Bokyoung Kim , Sebastien Lépine

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 new $P -\phi_{31}-{\rm [Fe/H]}$ and $P -\phi_{31}- A_2 - {\rm [Fe/H]}$ relations for fundamental-mode (RRab) and first-overtone mode (RRc) RR Lyrae stars (RRLs), respectively. The relations were calibrated based on pulsation…

太阳与恒星天体物理 · 物理学 2024-07-09 Tatiana Muraveva , Andrea Giannetti , Gisella Clementini , Alessia Garofalo , Lorenzo Monti

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

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

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…

星系天体物理 · 物理学 2020-10-14 Hangci Du , Shude Mao , E. Athanassoula , Juntai Shen , Pawel Pietrukowicz

We characterize the spatial density of the Pan-STARRS1 (PS1) sample of RR Lyrae stars, to study the properties of the old Galactic stellar halo as traced by RRab stars. This sample of 44,403 sources spans Galactocentric radii of $0.55 \;…

Based on a large spectroscopic sample of $\sim$ 4,300 RR Lyrae stars with metallicity, systemic radial velocity and distance measurements, we present a detailed analysis of the chemical and kinematic properties of the Galactic halo. Using…

星系天体物理 · 物理学 2022-09-28 Gaochao Liu , Yang Huang , Sarah Ann Bird , Huawei Zhang , Fei Wang , Haijun Tian

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…

星系天体物理 · 物理学 2020-01-08 R. Zinn , X. Chen , A. C. Layden , D. I. Casetti-Dinescu

We present a RR Lyrae (RRL) catalogue based on the combination of the third data release of the Zwicky Transient Facility (ZTF DR3) and \textit{Gaia} EDR3. We use a multi-step classification pipeline relying on the Fourier decomposition…

星系天体物理 · 物理学 2021-12-22 Kuan-Wei Huang , Sergey E. Koposov

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…

星系天体物理 · 物理学 2026-04-29 T. Muraveva , L. Monti , D. Massari , M. De Leo , A. Garofalo , G. Clementini , E. Ceccarelli , U. Michelucci
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