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相关论文: MN112: a new Galactic candidate Luminous Blue Vari…

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We discuss moderate resolution spectra, multicolor photometry, and light curves of thirty-one of the most luminous stars and variables in the giant spiral M101. The majority are intermediate A to F-type supergiants. We present new…

太阳与恒星天体物理 · 物理学 2015-06-23 Skyler H. Grammer , Roberta M. Humphreys , Jill Gerke

We search for LBV stars in galaxies outside the Local Group. Here we present a study of two bright $H\alpha$ sources in the NGC 247 galaxy. Object j004703.27-204708.4 ($M_V=-9.08 \pm 0.15^m$) shows the spectral lines typical for…

太阳与恒星天体物理 · 物理学 2020-09-02 Y. Solovyeva , A. Vinokurov , A. Sarkisyan , K. Atapin , S. Fabrika , A. F. Valeev , A. Kniazev , O. Sholukhova , O. Maslennikova

Luminous blue variables (LBVs) are expected to play an important role in massive stellar evolution as well as being the progenitors of some of the most luminous supernovae known. In this paper we provide a multiwavelength study of the…

太阳与恒星天体物理 · 物理学 2015-06-04 J. S. Clark , N. Castro , M. Garcia , A. Herrero , F. Najarro , I. Negueruela , B. W. Ritchie , K. T. Smith

Massive evolved stars loss a large fraction of their mass via copious stellar wind or instant outbursts and during certain evolutionary phases they can be identified via the presence of their circumstellar nebulae. In this paper, we present…

太阳与恒星天体物理 · 物理学 2015-05-14 V. V. Gvaramadze , A. Y. Kniazev , S. Fabrika

We report optical and near-infrared spectra of the central star of the radio source G79.29+0.46, a candidate luminous blue variable. The spectra contain numerous narrow (FWHM < 100 km/s emission lines of which the low-lying hydrogen lines…

天体物理学 · 物理学 2007-05-23 R. H. M. Voors , T. R. Geballe , L. B. F. M. Waters , F. Najarro , H. J. G. L. M. Lamers

We report time-series photometry for 16 variable stars located in the central part of the globular cluster NGC 6752. The sample includes 13 newly identified objects. The precision of our differential photometry ranges from 1 mmag at V=14.0…

太阳与恒星天体物理 · 物理学 2014-11-20 Janusz Kaluzny , Ian B. Thompson

In the current paper, we present a study of the spatial distribution of luminous blue variables (LBVs) and various LBV candidates (cLBVs) with respect to OB associations in the M33 galaxy. The identification of blue star groups was based on…

We report the discovery of a circular mid-infrared shell around the emission-line star Wray 16-137 using archival data of the Spitzer Space Telescope. Follow-up optical spectroscopy of Wray 16-137 with the Southern African Large Telescope…

太阳与恒星天体物理 · 物理学 2015-06-22 V. V. Gvaramadze , A. Y. Kniazev , L. N. Berdnikov , N. Langer , E. K. Grebel , J. M. Bestenlehner

The luminous blue variable (LBV) RMC143 is located in the outskirts of the 30~Doradus complex, a region rich with interstellar material and hot luminous stars. We report the $3\sigma$ sub-millimetre detection of its circumstellar nebula…

An increasing number of non-terminal eruptions are being found in the numerous surveys for optical transients. Very little is known about these giant eruptions, their progenitors and their evolutionary state. A greatly improved census of…

太阳与恒星天体物理 · 物理学 2015-06-22 Roberta M. Humphreys , Kerstin Weis , Kris Davidson , D. J. Bomans , Birgitta Burggraf

We perform a study on the optical and infrared photometric properties of known luminous blue variables (LBVs) in M31 using the sample of LBV candidates from the Local Group Galaxy Survey (Massey et al. 2007). We find that M31 LBV candidates…

We present two new luminous blue variable (LBV) candidate stars discovered in the M33 galaxy. We identified these stars (Valeev et al. 2010) as massive star candidates at the final stages of evolution, presumably with a notable interstellar…

太阳与恒星天体物理 · 物理学 2015-05-19 A. F. Valeev , O. N. Sholukhova , S. N. Fabrika

Context. Luminous blue variables (LBVs) are rare massive stars with very high luminosity. They are characterized by strong photo-metric and spectroscopic variability related to transient eruptions. The mechanisms at the origin of these…

Luminous Blue Variables (LBVs) are massive stars that are likely to be a transitionary phase between O stars and hydrogen-free classical Wolf-Rayet stars. The variability of these stars has been an area of study for both professional and…

The field of the globular cluster M22 (NGC 6656) was monitored between 2000 and 2008 in a search for variable stars. $BV$ light curves were obtained for 359 periodic, likely periodic, and long-term variables, 238 of which are new…

太阳与恒星天体物理 · 物理学 2018-10-24 M. Rozyczka , I. B. Thompson , W. Pych , W. Narloch , R. Poleski , A. Schwarzenberg-Czerny

Searches for compact mid-IR nebulae with the Spitzer Space Telescope and the Wide-field Infrared Survey Explorer (WISE), accompanied by spectroscopic observations of central stars of these nebulae led to the discovery of many dozens of…

太阳与恒星天体物理 · 物理学 2016-11-07 V. V. Gvaramadze , A. Y. Kniazev

A total of 185 luminous blue variable (LBV) candidates with V < 18.5 and B-V < 0.35 are selected based on the photometrical Survey of Local Group Galaxies made by P. Massey et al. 2006. The candidates were selected using aperture photometry…

太阳与恒星天体物理 · 物理学 2015-05-19 A. F. Valeev , O. Sholukhova , S. Fabrika

We present the results of spectroscopy and multi-wavelength photometry of luminous and variable star candidates in the nearby spiral galaxies NGC 2403 and M81. We discuss specific classes of stars, the Luminous Blue Variables (LBVs), B[e]…

太阳与恒星天体物理 · 物理学 2019-01-09 Roberta M. Humphreys , Sarah Stangl , Michael S. Gordon , Kris Davidson , Skyler H. Grammer

Recent IR surveys of the Galactic plane have revealed a large number of candidate Luminous Blue Variables. In order to verify these classifications we have been undertaking a long term spectroscopic and photometric monitoring campaign…

太阳与恒星天体物理 · 物理学 2010-12-15 J. S. Clark , A. Arkharov , V. Larionov , B. Ritchie , P. Crowther , F. Najarro

We describe a search for H-alpha emission-lined stars in M31, M33, and seven dwarfs in or near the Local Group (IC 10, NGC 6822, WLM, Sextans B, Sextans A, Pegasus and the Phoenix dwarf) using interference filter imaging with the KPNO and…