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The recent discovery, based on a search of public OGLE data, of Be star candidates in the Small Magellanic Cloud showing spectacular photometric variations (Mennickent et al. 2002), has motivated further analysis of their light curves. Here…

Astrophysics · Physics 2007-05-23 R. E. Mennickent , G. Pietrzynski , W. Gieren

Detailed studies of Be stars in environments with different metallicities like the Magellanic Clouds or the Galactic bulge are necessary to understand the formation and evolution mechanisms of the circumstellar disks. However, a detailed…

Astrophysics · Physics 2009-11-13 B. E. Sabogal , R. E. Mennickent , G. Pietrzyński , J. A. García , W. Gieren , Z. Kolaczkowski , .

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…

Astrophysics · Physics 2009-11-10 W. J. de Wit , J-P. Beaulieu , H. J. G. L. M. Lamers , E. Lesquoy , J-B. Marquette , ;

We present a variability study of 4646 massive stars in the Small Magellanic Cloud (SMC) with known spectral types from the catalog of Bonanos et al. (2010) using the light curves from the OGLE-III database. The goal is to exploit the time…

We present a proper motion investigation of a sample of Be star candidates towards the Magellanic Clouds, which has resulted in the identification of separate populations, in the Galactic foreground and in the Magellanic background. Be…

Astrophysics of Galaxies · Physics 2017-06-28 Katherine Vieira , Alejandro García-Varela , Beatriz Sabogal

We report on the study of the population of B and Be stars in SMC young clusters, performed with the Wide Field Imager in slitless spectroscopic mode at ESO/T2.2m with a filter centered at Halpha. First, we explain the reduction methods we…

(Abridged) Some 240 blue stars in the Small Magellanic Cloud are investigated on their fantastic irregular continuum variability. We report here two results regarding these stars. First, their optical flux excess is correlated to their…

Astrophysics · Physics 2009-11-11 W. J. de Wit , H. J. G. L. M. Lamers , J. B. Marquette , J. P. Beaulieu , ;

We present the results of a search for Be stars in six fields centered on the young clusters NGC 330 and NGC 346 in the SMC, and NGC 1818, NGC 1948, NGC 2004 and NGC 2100 in the LMC. Be stars were identified by differencing R band and…

Astrophysics · Physics 2009-10-30 Stefan C Keller , Peter R Wood , Michael S Bessell

We present a study of the infrared properties of 4922 spectroscopically confirmed massive stars in the Large and Small Magellanic Clouds, focusing on the active OB star population. Besides OB stars, our sample includes yellow and red…

The eighth part of the OGLE-III Catalog of Variable Stars (OIII-CVS) contains type II Cepheids in the Small Magellanic Cloud (SMC). The sample consists of 43 objects, including 17 BL Her, 17 W Vir and 9 RV Tau stars (first examples ever…

Solar and Stellar Astrophysics · Physics 2010-07-16 I. Soszynski , A. Udalski , M. K. Szymanski , M. Kubiak , G. Pietrzynski , L. Wyrzykowski , K. Ulaczyk , R. Poleski

We present the results of a photometric survey for Be stars in eleven young clusters in the Large Magellanic Cloud and fourteen young clusters in the Small Magellanic Cloud. B stars with hydrogen in emission are identified on the basis of…

Astrophysics of Galaxies · Physics 2015-06-17 Shaheen Iqbal , Stefan C. Keller

Multi-color OGLE survey light curves of about 20 years duration are analyzed for about 3000 classical Be stars in the Large and Small Magellanic Clouds (LMC, SMC) in order to study the properties and variability. Each light curve was…

Solar and Stellar Astrophysics · Physics 2025-05-14 A. L. Figueiredo , A. C. Carciofi , J. Labadie-Bartz , M. L. Pinho , T. H. de Amorin , P. T. dos Santos , I. Soszyński , A. Udalski

Mennickent et al.and Sabogal et al.identified a large number of Classical Be (CBe) candidates in the L&SMC based on their photometric variability using the OGLEII database. They classified these stars into four different groups based on the…

Solar and Stellar Astrophysics · Physics 2015-06-04 K. T. Paul , A. Subramaniam , B. Mathew , R. E. Mennickent , B. Sabogal

As part of an ongoing photometric survey of young Magellanic Cloud clusters we identified Be stars in NGC 1818 and a nearby smaller cluster in the Large Magellanic Cloud. The neighbouring cluster does not contain evolved stars, and its…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Eva K. Grebel

We present period-luminosity relations for more than 3,200 red variable stars in the Small Magellanic Cloud observed in the second phase of the Optical Gravitational Lensing Experiment (OGLE-II). Periods of multiply-periodic light curve…

Astrophysics · Physics 2009-11-10 L. L. Kiss , T. Bedding

We present a collection of 991 heartbeat star (HBS) candidates found in the Optical Gravitational Lensing Experiment (OGLE) project data archive. We discuss the selection process of the HBS candidates and the structure of the catalog…

We observed a large sample of B & Be stars in the Magellanic Clouds, respectively 176 and 344 stars, with the multi-object spectrograph GIRAFFE at ESO/VLT. We obtained spectra at different settings at various epochs. It allowed us to…

Astrophysics · Physics 2007-05-23 Christophe Martayan , Michele Floquet , Anne-Marie Hubert , Malek Mekkas

We revisit the subject of Be star candidates towards the Magellanic Clouds, previously studied by the authors using SPM4 proper motions. We obtain GAIA DR2 parallaxes and proper motions for 2357 and 994 LMC and SMC Be candidates,…

Solar and Stellar Astrophysics · Physics 2021-06-09 Katherine Vieira , Alejandro García-Varela , Beatriz Sabogal , Leandro Rocha Rímulo , Jesús Hernández

Using data from the EROS2 microlensing survey, we report the discovery of two blue objects with irregular photometric behaviour of $\Delta V \sim 0.1$-0.4 mag on time scales of 20 to 200 days. They show a bluer when fainter behaviour.…

We present the first-ever collection of delta Scuti stars found over the entire area of the Small Magellanic Cloud (SMC). The sample consists of 2810 variables of which over 2600 objects belong to the SMC while the remaining stars are most…

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