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相关论文: New Oe stars in LAMOST DR5

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We report the discovery of 5 new Herbig Ae/Be candidate stars in the Small Magellanic Cloud in addition to the 2 reported in Beaulieu et al. (2001). We discuss these 7 HAeBe candidate stars in terms of (1) their irregular photometric…

天体物理学 · 物理学 2009-11-10 W. J. de Wit , J-P. Beaulieu , H. J. G. L. M. Lamers , E. Lesquoy , J-B. Marquette , ;

We present the first stellar spectroscopy in the low-luminosity (M_V ~-9.3 mag), dwarf galaxy Leo P. Its significantly low oxygen abundance (3% solar) and relative proximity (~1.6 Mpc) make it a unique galaxy to investigate the properties…

We briefly discuss three cases of RR~Lyrae variable stars with Blazhko modulation from the OGLE Galactic bulge collection. In one of the discussed stars modulation with two periods is detected, in other star, we detect three Blazhko…

太阳与恒星天体物理 · 物理学 2016-01-12 Karolina Bakowska , Radoslaw Smolec

We identify the RR Lyrae and delta Scuti (DSCT) stars in three catalogs of GALEX variable sources. The NUV amplitude of RR Lyrae stars is about twice that in V-band, so we find a larger percentage of low amplitude variables than catalogs…

太阳与恒星天体物理 · 物理学 2015-06-22 T. D. Kinman , Warren R. Brown

We performed the slitless spectroscopic survey to identify Classical (CBe) stars in open clusters older than 100 Myr. Observing a sample of 71 open clusters, we identified 13 CBe stars in 11 open clusters, one of, which (TYC 2679-432-1) is…

太阳与恒星天体物理 · 物理学 2022-04-04 Madhu Kashyap Jagadeesh , Blesson Mathew , K. T. Paul , Gourav Banerjee , Annapurni Subramaniam , R. Arun

Oe stars possibly form an extension to higher temperatures of the Be phenomenon, but it is still unclear whether these stars have disks. X-ray spectra could provide hints for interactions of the star with a putative surrounding disk. We…

太阳与恒星天体物理 · 物理学 2020-12-09 G. Rauw , Y. Naze , M. Spano , T. Morel , A. ud-Doula

Our new survey for Wolf-Rayet stars in the Magellanic Clouds is only 15% complete but has already found 9 new WRs in the LMC. This suggests that the total WR population in the LMC may be underestimated by 10-40%. Eight of the nine are WNs,…

太阳与恒星天体物理 · 物理学 2015-06-22 Philip Massey , Kathryn F. Neugent , Nidia Morrell , D. John Hillier

Rare types of variable star may give unique insight into short-lived stages of stellar evolution. The systematic monitoring of millions of stars and advanced light curve analysis techniques of microlensing surveys make them ideal for…

AST3-1 is the second-generation wide-field optical photometric telescope dedicated to time domain astronomy at Dome A, Antarctica. Here we present the results of $i$ band images survey from AST3-1 towards one Galactic disk field. Based on…

We present the results of a search for pulsating stars in the 7.12 deg^2 OGLE-III Galactic disk area in the direction tangent to the Centaurus Arm. We report the identification of 20 Classical Cepheids, 45 RR Lyr type stars, 31 Long-Period…

We present the analysis of the top-quality photometry of RR Lyrae stars in the globular cluster NGC 6362, gathered over 11 observing seasons by the CASE project. 16 stars are fundamental mode pulsators (RRab stars) and 16 are first overtone…

太阳与恒星天体物理 · 物理学 2017-02-28 R. Smolec , P. Moskalik , J. Kaluzny , W. Pych , M. Rozyczka , I. B. Thompson

Based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) medium-resolution spectroscopic survey (MRS), we report the discovery of nine super Li-rich unevolved stars with A(Li) $>$ 3.8 dex. These objects show unusually…

太阳与恒星天体物理 · 物理学 2022-04-20 T. -S. Yan , J. -R. Shi , L. Wang , H. -L. Yan , Z. -M. Zhou , Y. -T. Zhou , X. -S. Fang , C. -Q. Li , T. -Y. Chen , X. -J. Xie

We present new large samples of Galactic Cepheids and RR Lyrae stars from the OGLE Galaxy Variability Survey.

太阳与恒星天体物理 · 物理学 2017-09-13 Andrzej Udalski

Based on the first Gaia data release and spectroscopy from the LAMOST Data Release 4, we study the kinematics and chemistry of the local halo stars. The halo stars are identified kinematically with a relative speed of at least 220 km…

星系天体物理 · 物理学 2018-08-22 Cuihua Du , Hefan Li , Shuai Liu , Thomas Donlon , Heidi Jo Newberg

We report the detection of 1143 variable stars towards the Galactic bulge, including 320 previously uncatalogued variables, using time-series photometry extracted from data obtained with the VIMOS imager at the Very Large Telescope.…

太阳与恒星天体物理 · 物理学 2018-10-31 N. Kains , A. Calamida , M. Rejkuba , A. Bhardwaj , L. Inno , K. C. Sahu , M. Zoccali , G. Bono , F. Surot , J. Anderson , S. Casertano

We study a sample of 14 spectroscopically confirmed Ly$\alpha$ Emitters (LAEs) in the late era of reionization (at redshift $z\approx6$) based on the JWST/NIRCam imaging dataset. These LAEs with high Ly$\alpha$ luminosity of $L$(Ly$\alpha$)…

This study utilized LAMOST low-resolution spectra to identify M-type YSOs and characterize their accretion signatures. We measured characteristic features, including hydrogen Balmer, Li {\sc i}, He~{\sc i}, Na {\sc i}, and Ca {\sc ii}…

太阳与恒星天体物理 · 物理学 2025-05-20 Xiang-Song Fang , Jian-Rong Shi , Ming-Yi Ding , Zi-Huang Cao

We have undertaken a near-IR spectral survey of stars associated with compact nebulae recently revealed by the Spitzer and WISE imaging surveys. These circumstellar nebulae, produced by massive evolved stars, display a variety of symmetries…

星系天体物理 · 物理学 2011-12-13 G. S. Stringfellow , V. V. Gvaramadze , Y. Beletsky , A. Y. Kniazev

We analyze longslit spectral observations of fourteen Wolf-Rayet galaxies from the sample of Schaerer, Contini & Pindao (1999). All 14 galaxies show broad Wolf-Rayet emission in the blue region of the spectrum, consisting of a blend of…

天体物理学 · 物理学 2009-11-10 I. F. Fernandes , R. de Carvalho , T. Contini , R. R. Gal

Using an image subtraction method we have searched for variable stars in the globular cluster M14. We confirmed 62 previously known catalogued variables. In addition to the previoulsy known variables we have identified 71 new variables. We…

太阳与恒星天体物理 · 物理学 2012-05-15 Kyle E. Conroy , Andrew N. Darragh , Zheyu J. Liu , Brian W. Murphy
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