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We present the analyses of the stellar contents associated with the HII region Sh2-252 using UBVRI photometry, slit and slitless spectroscopy along with the NIR data from 2MASS for an area ~1 degree x 1 degree. We studied the sub-regions of…

Solar and Stellar Astrophysics · Physics 2013-01-01 Jessy Jose , A. K. Pandey , K. Ogura , M. R. Samal , D. K. Ojha , B. C. Bhatt , N. Chauhan , C. Eswaraiah , H. Mito , N. Kobayashi , R. K. Yadav

We present an updated catalog of 1300 objects in the field of M31, including 670 likely star clusters of various types. Archival images were inspected to confirm cluster classifications where possible, but most of the classifications were…

We present the results of the first broadband 10.8 um survey of the NGC 2024 cluster. The mid-infrared data were combined with our previously published JHKL photometry in order to construct spectral energy distributions for all detected…

We employed the ESO MPI wide-field camera and obtained deep images in the VIc pass-bands in the region of the IC 2944/2948 complex (l ~ 294; b ~ -1), and complemented them with literature and archival data. We used this material to derive…

Solar and Stellar Astrophysics · Physics 2015-06-19 G. Baume , M. J. Rodríguez , M. A. Corti , G. Carraro , J. A. Panei

We have used a combination of high-resolution Hubble Space Telescope WFPC2 and wide-field ground-based observations, in ultraviolet and optical bands, to study the blue straggler star population of the massive outer-halo globular cluster…

Astrophysics of Galaxies · Physics 2013-11-07 N. Sanna , E. Dalessandro , F. R. Ferraro , B. Lanzoni , P. Miocchi , R. W. O'Connell

Young star clusters consisting of massive stars are the ideal sites to study the star formation processes and influence of massive stars on the subsequent star formation. NGC 1893 is a young star cluster associated with the HII region…

Solar and Stellar Astrophysics · Physics 2022-02-09 Neelam Panwar , Amit Kumar , S. B. Pandey

We present a comprehensive study of massive young stellar objects (YSOs) in the metal-poor galaxy NGC 6822 using IRAC and MIPS data obtained from the {\em Spitzer Space Telescope}. We find over 500 new YSO candidates in seven massive…

Astrophysics of Galaxies · Physics 2019-09-25 Olivia C. Jones , Michael J. Sharp , Megan Reiter , Alec S. Hirschauer , M. Meixner , Sundar Srinivasan

We report the properties of a new young double stellar cluster in the region towards IRAS 07141-0920 contained in the HII region Sh2-294. High-resolution optical UBVRI and Halpha images, near-infrared JHKs and H2 filter images were used to…

Astrophysics · Physics 2009-11-13 Joao L. Yun , Anlaug Amanda Djupvik , Antonio J. Delgado , Emilio J. Alfaro

We report the outcome of a deep multi-wavelength study of the IC2391 young open cluster. We aim at uncovering new low-mass and sub-stellar members of the cluster and identifying new debris disk objects. A 30*30 square arcmin area in IC 2391…

Solar and Stellar Astrophysics · Physics 2015-05-13 L. Spezzi , I. Pagano , G. Marino , G. Leto , E. Young , N. Siegler , Z. Balog , S. Messina , E. Distefano , B. Merin , D. Barrado y Navascues

We report a study of the stellar content of the Near-infrared cluster [DBS2003]\,157 embedded in the extended H\,{\sc ii} region GAL\,331.31-00.34, which is associated with the IRAS source 16085-5138. $JHK$ photometry was carried out in…

We studied the star cluster population properties in the nearby collisional ring galaxy NGC 922 using HST/WFPC2 photometry and population synthesis modeling. We found that 69% of the detected clusters are younger than 7 Myr, and that most…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Anne Pellerin , Gerhardt R. Meurer , Kenji Bekki , Debra M. Elmegreen , O. Ivy. Wong , Patricia Knezek

NGC 5822 is a richly populated, moderately nearby, intermediate-age open cluster covering an area larger than the full moon on the sky. A CCD survey of the cluster on the UBVI and uvbyCaHbeta systems shows that the cluster is superposed…

Solar and Stellar Astrophysics · Physics 2015-05-30 Giovanni Carraro , Barbara J. Anthony-Twarog , Edgardo Costa , Bryce J. Jones , Bruce A. Twarog

We present a study of the spatial distribution of the stellar cluster populations in the star forming galaxy NGC 628. Using Hubble Space Telescope broad band WFC3/UVIS UV and optical images from the Treasury Program LEGUS (Legacy…

We performed a HST/WFC3-IR imaging survey of the young stellar cluster NGC 2024 in three filters probing the 1.4~$\mu$m H$_2$O absorption feature, characteristic of the population of low mass and sub-stellar mass objects down to a few…

(abridged) NGC6530 is a young cluster with a complex morphology and star-formation history. We present a statistical study of its global properties using a new large list of candidate members down to masses of 0.2-0.4 Msun and Gaia DR2…

Solar and Stellar Astrophysics · Physics 2019-02-27 F. Damiani , L. Prisinzano , G. Micela , S. Sciortino

The nearby dwarf starburst galaxy NGC5253 hosts a number of young, massive star clusters, the two youngest of which are centrally concentrated and surrounded by thermal radio emission (the `radio nebula'). To investigate the role of these…

{Aims.} We introduce our imaging survey of possible young massive globular clusters in M31 performed with the Wide Field and Planetary Camera 2 (WFPC2) on the Hubble Space Telescope (HST). We present here details of the data reduction…

IRAS 12272-6240 is a complex star forming region with a compact massive dense clump and several associated masers, located at a well-determined distance of $d=9.3$ kpc from the Sun. For this study, we obtained sub-arcsec broad- and…

Astrophysics of Galaxies · Physics 2020-06-29 Mauricio Tapia , Paolo Persi , Miguel Roth , Davide Elia

We present $UBVI_c$ CCD photometry of the young open cluster Stock 8 with the aim to study the basic properties and star formation scenario in this region. The radius of the cluster is found to be $\sim 6^{\prime}$ ($\sim 3.6$ pc) and the…

NGC 2264 is a young Galactic cluster and the dominant component of the Mon OB1 association lying approximately 760 pc distant within the local spiral arm. The cluster is hierarchically structured, with subclusters of suspected members…

Astrophysics · Physics 2008-08-29 S. E. Dahm