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We present a radial velocity analysis of 20 solar neighborhood RR Lyrae and 3 Population II Cepheids variables. We obtained high-resolution, moderate-to-high signal-to-noise ratio spectra for most stars and obtained spectra were covering…

太阳与恒星天体物理 · 物理学 2017-11-16 N. E. Britavskiy , E. Pancino , V. Tsymbal , D. Romano , L. Fossati

We present a group of 3740 previously identified RR Lyrae variables well-observed with the Wide-field Infrared Survey Explorer (WISE). We explore how the shape of the generic RR Lyrae mid-infrared light curve evolves in period-space,…

太阳与恒星天体物理 · 物理学 2015-06-18 Tatyana Gavrilchenko , Christopher R. Klein , Joshua S. Bloom , Joseph W. Richards

The intensities of the hydrogen Balmer lines of solar-like stars are investigated for stellar chromospheric activity by using the co-source spectral data of the LAMOST Low-Resolution Spectroscopic Survey (LRS) and Medium-Resolution…

太阳与恒星天体物理 · 物理学 2024-08-06 Han He

Modern theories of galaxy formation predict that the Galactic stellar halo was hierarchically assembled from the accretion and disruption of smaller systems. This hierarchical assembly is expected to produce a high degree of structure in…

We present preliminary results of H_alpha near-infrared spectroscopy of six galaxies with redshifts z ~ 1 drawn from the DEEP2 Galaxy Redshift Survey. The spectra have been taken with the multi-slit mode of LIRIS (Long-slit Intermediate…

RV variable stars are important in astrophysics. The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) spectroscopic survey has provided ~ 6.5 million stellar spectra in its Data Release 4 (DR4). During the survey, ~ 4.7…

We determine the period-magnitude relations of RR Lyrae stars in 13 photometric bandpasses from 0.4 to 12 {\mu}m using timeseries observations of 134 stars. The Bayesian formalism, extended from our previous work to include the effects of…

太阳与恒星天体物理 · 物理学 2014-06-10 Christopher R. Klein , Joshua S. Bloom

We present the first results of a spectroscopic survey of Lyman break galaxies in the near-infrared aimed at detecting the emission lines of [O II], [O III], and Hbeta from the H II regions of star forming galaxies at z = 3. From…

LAMOST DR5 released more than 200,000 low resolution spectra of early-type stars with S/N>50. Searching for metallic-line (Am) stars in such a large database and study of their statistical properties are presented in this paper. Six machine…

太阳与恒星天体物理 · 物理学 2019-06-05 Li Qin , A-Li Luo , Wen Hou , Yin-Bi Li , Shuo Zhang , Rui Wang , Li-Li Wang , Xiao Kong , Jin-Shu Han

The evolution of the universe together with the galaxies is one of the fundamental issues that we humans are most interested in. Both the observations of tidal streams from SDSS and the theory of $\Lambda$CDM support the hierarchical…

星系天体物理 · 物理学 2025-04-16 Yanhui Chen

We present the detection of 6,371 RR Lyrae (RRL) stars distributed across ~14,000 deg^2 of the sky from the combined data of the Sloan Digital Sky Survey (SDSS), the Panoramic Survey Telescope and Rapid Response System 1 (PS1), and the…

星系天体物理 · 物理学 2015-06-19 M. A. Abbas , E. K. Grebel , N. F. Martin , W. S. Burgett , H. Flewelling , R. J. Wainscoat

As part of the LAMOST medium-resolution spectroscopic survey, the LAMOST-MRS-O is a non-time domain survey that aims to perform medium-resolution spectral observations for member stars in the open cluster area. This survey plans to obtain…

星系天体物理 · 物理学 2025-01-16 Xi Zhang , Chengzhi Liu , Jing Zhong , Li Chen , Ali Luo , Jian-Rong Shi , Chao Liu , JianJun Chen , Haotong Zhang , Jinliang Hou

The space photometric project "Lyra" is developed now in Russia.The project purpose is determination of the photometric information and coordinates of the natural and artificial space objects, from the brightest ones to 16^m in visual…

天体物理仪器与方法 · 物理学 2010-02-26 Alexey V. Mironov , Andrey I. Zakharov , Mikhail E. Prokhorov , Feodor N. Nikolaev , Maxim N. Tuchin

Oxygen is a powerful tracer element of Galactic chemical evolution. Unfortunately, only a few oxygen lines are available in the ultraviolet-infrared stellar spectra for the reliable determination of its abundance. Moreover, oxygen…

太阳与恒星天体物理 · 物理学 2014-09-11 A. Kucinskas , V. Dobrovolskas , P. Bonifacio , E. Caffau , H. -G. Ludwig , M. Steffen , M. Spite

The recent precise photometric observations and successes of the modelling efforts transformed our picture of the pulsation of RR Lyrae stars. The discovery of additional frequencies and the period doubling phenomenon revealed that a…

太阳与恒星天体物理 · 物理学 2015-06-16 E. Plachy , Z. Kolláth , L. Molnár

We discuss a sample of over 3000 candidate RR Lyrae stars selected by various methods using Sloan Digital Sky Survey data for about 1000 deg^2 of sky. These stars probe the halo structure out to ~100 kpc from the Galactic center. Their…

RR Lyrae stars in the Milky Way are good tracers to study the kinematic behaviour and spatial distribution of older stellar populations. A recently established well documented sample of 217 RR Lyr stars with V<12.5 mag, has been used to…

天体物理学 · 物理学 2009-11-11 Gisela Maintz , Klaas S. de Boer

Deep near-IR images from the VISTA Variables in the V\'ia L\'actea (VVV) Survey were used to search for RR Lyrae stars in the Southern Galactic plane. A sizable sample of 404 RR Lyrae of type ab stars was identified across a thin slice of…

RR Lyrae stars being distance indicators and tracers of old population serve as excellent probes of the structure, formation, and evolution of our Galaxy. Thousands of them are being discovered in ongoing wide-field surveys. The OGLE…

星系天体物理 · 物理学 2016-09-07 Pawel Pietrukowicz , OGLE collaboration

We present observations of eleven compact star-forming galaxies in the redshift range z = 0.6145 - 1.0053, with the Cosmic Origins Spectrograph (COS) on board the Hubble Space Telescope (HST). We aim to spectroscopically measure for the…

星系天体物理 · 物理学 2025-10-28 Y. I. Izotov , D. Schaerer , G. Worseck , N. G. Guseva , A. Verhamme , C. Simmonds , J. Chisholm