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Related papers: Young open clusters in the Milky Way and Small Mag…

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We present a catalogue of new spectral types for hot, luminous stars in the Small Magellanic Cloud. The catalogue contains 4161 objects, giving an order of magnitude increase in the number of SMC stars with published spectroscopic…

Astrophysics · Physics 2014-10-13 C. J. Evans , I. D. Howarth , M. J. Irwin , A. W. Burnley , T. J. Harries

We have recalculated the orbits of 3 binary systems, members of the open cluster Trumpler 16 in the Carina region. We have added new observations to those available in the literature. Also, we have also tried to find the orbital periods for…

Astrophysics · Physics 2007-05-23 G. J. Luna , H. Levato , S. Malaroda , M. Grosso

(Abridged) The open cluster NGC 1893, illuminating the HII region IC410, contains a moderately large population of O-type stars and is one of the youngest clusters observable in the optical range. We have probed the stellar population of…

Astrophysics · Physics 2011-04-19 Ignacio Negueruela , Amparo Marco , GianLuca Israel , Guillem Bernabeu

We present new version of the OGLE-II catalog of eclipsing binary stars detected in the Small Magellanic Cloud, based on Difference Image Analysis catalog of variable stars in the Magellanic Clouds containing data collected from 1997 to…

The new census of massive stars in the Carina nebula reveals the presence of 54 apparently single O-type stars in the Car OB1 association, an extremely active star-forming region which hosts some of the most luminous stars of the Milky Way.…

Aims. We analyze the population of periodic variable stars in the open cluster NGC 3766 based on a 7-year multi-band monitoring campaign conducted on the 1.2 m Swiss Euler telescope at La Silla, Chili. Methods. The data reduction, light…

Solar and Stellar Astrophysics · Physics 2015-06-15 N. Mowlavi , F. Barblan , S. Saesen , L. Eyer

We present here the results of our research for B-type pulsators in low metallicity environments, searching for short-term periodic variability in a large sample of B and Be stars in the Magellanic Clouds (MC), for which the fundamental…

Solar and Stellar Astrophysics · Physics 2009-02-26 P. D. Diago , J. Gutiérrez-Soto , J. Fabregat , C. Martayan

We present observations for three star clusters, Kron 11, Kron 63 and NGC 121, in the Small Magellanic Cloud. We have studied their structure and derived their fundamental parameters by means of their luminosity functions, their color…

Astrophysics · Physics 2016-09-08 G. Baume , N. E. D. Noël , E. Costa , G. Carraro , R. A. Méndez , M. H. Pedreros

M16=NGC 6611, the Eagle Nebula, is a well studied region of star formation and the source of a widely recognized Hubble Space Telescope (HST) image. High spatial resolution infrared observations with the Near Infrared Camera and…

Astrophysics · Physics 2010-12-23 Rodger I. Thompson , Bradford A. Smith , J. Jeff Hester

Multiple stellar populations (MPs) representing star-to-star light-element abundance variations are common in nearly all ancient Galactic globular clusters. Here we provide the strongest evidence yet that the populous, ~ 1.7 Gyr-old Large…

Astrophysics of Galaxies · Physics 2022-03-14 Shalmalee Kapse , Richard de Grijs , Devika Kamath , Daniel B. Zucker

We consider the possibility of cluster membership for 13 planetary nebulae that are located in close proximity to open clusters lying in their lines of sight. The short lifetimes and low sample size of intermediate-mass planetary nebulae…

Astrophysics · Physics 2009-11-13 Daniel J. Majaess , David G. Turner , David J. Lane

Only four globular cluster planetary nebulae (GCPN) are known so far in the Milky Way. About 50 new globular clusters have been recently discovered towards the Galactic bulge. We present a search for planetary nebulae within 3 arcmin of the…

Solar and Stellar Astrophysics · Physics 2019-10-16 Dante Minniti , Bruno Dias , Matías Gómez , Tali Palma , Joyce B. Pullen

The Magellanic Clouds offer a unique variety of star forming regions seen as bright nebulae of ionized gas, related to bright young stellar associations. Nowadays, observations with the high resolving efficiency of the Hubble Space…

Astrophysics · Physics 2009-11-13 Dimitrios A. Gouliermis

The detection of magnetic chemically peculiar (CP2) stars in open clusters of extragalactic systems can give observational answers to many unsolved questions. The mean percentage of CP2 stars in the Milky Way is of the order of 5% for the…

Astrophysics · Physics 2009-11-11 E. Paunzen , H. M. Maitzen , O. I. Pintado , A. Claret , I. Kh. Iliev , M. Netopil

We present a multi-wavelength analysis of the star cluster NGC 2316 and its surroundings. We estimated the physical parameters of the NGC 2316 cluster, including its shape (elongated), size (Rcluster = 0.4 pc), distance (1.3 +/- 0.3 kpc),…

A large number of intermediate-age (~1-2-Gyr old) globular clusters (GCs) in the Large and the Small Magellanic Cloud (MC) exhibit either bimodal or extended main-sequence (MS) turn off and dual red clump. Moreover, recent papers have shown…

Solar and Stellar Astrophysics · Physics 2015-11-04 A. P. Milone

We report the discovery of 652 star clusters, stellar groups and candidates in the Milky Way with WISE. Most of the objects are projected close to Galactic Plane and are embedded clusters. The present sample complements a similar study…

Astrophysics of Galaxies · Physics 2015-12-03 Denilso Camargo , Eduardo Bica , Charles Bonatto

We present six new planetary nebulae (PNe) discovered in the Small Magellanic Cloud (SMC) from deep UK Schmidt telescope (UKST) narrow band Halpha and broad-band short-red "SR" continuum images and confirmed spectroscopically. These 6…

Astrophysics of Galaxies · Physics 2016-08-24 Danica Drašković , Quentin A. Parker , Warren A. Reid , Milorad Stupar

We present a multiwavelength study of the central part of the Carina Nebula, including Trumpler 16 and part of Trumpler 14. Analysis of the Chandra X-ray Observatory archival data led to the identification of nearly 450 X-ray sources. These…

The conventional picture of coeval, chemically homogeneous, populous star clusters -- known as `simple stellar populations' (SSPs) -- is a view of the past. Photometric and spectroscopic studies reveal that almost all ancient globular…

Astrophysics of Galaxies · Physics 2021-04-07 Shalmalee Kapse , Richard de Grijs , Daniel B. Zucker
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