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相关论文: Young Stellar Objects in NGC 6823

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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…

太阳与恒星天体物理 · 物理学 2015-05-30 Giovanni Carraro , Barbara J. Anthony-Twarog , Edgardo Costa , Bryce J. Jones , Bruce A. Twarog

W4 is a giant H{\sc ii} region ionized by the OB stars of the cluster IC~1805. The H{\sc ii} region/cluster complex has been a subject of numerous investigations as it is an excellent laboratory for studying the feedback effect of massive…

星系天体物理 · 物理学 2017-05-03 Neelam Panwar , M. R. Samal , A. K. Pandey , J. Jose , W. P. Chen , D. K. Ojha , K. Ogura , H. P. Singh , R. K. Yadav

We used archival Spitzer Space Telescope mid-infrared data to search for young stellar objects (YSOs) in the immediate vicinity of two bright-rimmed clouds, BRC 27 (part of CMa R1) and BRC 34 (part of the IC 1396 complex). These regions…

(Abridged) The chemical behaviour of an ample sample of PNe in NGC6822 is analyzed. Spectrophotometric data of 11 PNe and two H II regions were obtained with the OSIRIS spectrograph attached to the Gran Telescopio Canarias. Data for other…

星系天体物理 · 物理学 2016-01-27 Jorge García-Rojas , Miriam Peña , Sheila Flores-Durán , Liliana Hernández-Martínez

We present astrometry and $BVI$ photometry, down to $V\simeq22$, of the very young open cluster NGC6530, obtained from observations taken with the Wide Field Imager camera at the MPG/ESO 2.2 m Telescope. Both the $V$ vs. $B-V$ and the $V$…

天体物理学 · 物理学 2009-11-10 L. Prisinzano , F. Damiani , G. Micela , S. Sciortino

We describe a variability study of the moderately old open cluster NGC 6819. We have detected 4 new detached eclipsing binaries near the cluster turnoff (one of which may be in a triple system). Several of these systems should be able to…

太阳与恒星天体物理 · 物理学 2015-05-19 Antonio Talamantes , Eric L. Sandquist , James L. Clem , Russell M. Robb , David D. Balam , Matthew Shetrone

We present a UBV I and H alpha photometric study of the young open cluster NGC 1893 in the H II region W8 (IC 410 or Sh 2-236). A total of 65 early-type members are selected from photometric diagrams. A mean reddening of the stars is…

太阳与恒星天体物理 · 物理学 2015-06-19 Beomdu Lim , Hwankyung Sung , Jinyoung S. Kim , Michael S. Bessell , Byeong-Gon Park

Surface brightness profiles for 23 M31 star clusters were measured using images from the Wide Field Planetary Camera 2 on the Hubble Space Telescope, and fit to two types of models to determine the clusters' structural properties. The…

星系天体物理 · 物理学 2011-01-07 P. Barmby , S. Perina , M. Bellazzini , J. G. Cohen , P. W. Hodge , J. P. Huchra , M. Kissler-Patig , T. H. Puzia , J. Strader

The Wide-field Infrared Survey Explorer has uncovered a population of young stellar objects in the Western Circinus molecular cloud. Images show the YSOs to be clustered into two main groups that are coincident with dark filamentary…

太阳与恒星天体物理 · 物理学 2015-05-27 Wilson M. Liu , Deborah L. Padgett , David Leisawitz , Sergio Fajardo-Acosta , Xavier P. Koenig

We present a multiwavelength study of the Galactic H II region Sh2-297, located in Canis Major OB1 complex. Optical spectroscopic observations are used to constrain the spectral type of ionizing star HD 53623 as B0V. The classical nature of…

星系天体物理 · 物理学 2015-06-11 K. K. Mallick , D. K. Ojha , M. R. Samal , A. K. Pandey , B. C. Bhatt , S. K. Ghosh , L. K. Dewangan , M. Tamura

To date, the proposed observation of Young Stellar Objects (YSOs) in the Galactic center (GC) still raises the question where and how these objects could have formed due to the violent vicinity of Sgr~A*. Here, we report the…

We use deep images acquired with the Advanced Camera for Surveys (ACS) on board of the Hubble Space Telescope (HST) in the filters F555W and F814W to characterize the properties of NGC 376, a young star cluster located in the wing of the…

星系天体物理 · 物理学 2015-05-28 E. Sabbi , A. Nota , M. Tosi , L. J. Smith , J. Gallagher , M. Cignoni

We present star formation activity in the infrared dark cloud (IRDC) G53.2, a remarkable IRDC located at Galactic coordinates $(l,b)\sim(53^{\circ}.2,\,0^{\circ}.0)$ based on the census of young stellar object (YSO) candidates. IRDC G53.2…

星系天体物理 · 物理学 2015-06-23 Hyun-Jeong Kim , Bon-Chul Koo , Christopher J. Davis

Images obtained with the CTIO 4-m telescope and the MOSAIC-2 wide field camera in [O III] 5007 and H\alpha on-band and off-band filters are analyzed to search for emission lines objects in the galaxy NGC 6822. In particular we search for PN…

天体物理学 · 物理学 2009-11-13 Liliana Hernandez-Martinez , Miriam Pena

Stellar photometry derived from the INT/WFC Photometric H$\alpha$ Survey of the Northern Galactic Plane (IPHAS) can be used to identify large, reliable samples of A0-A5 dwarfs. For every A star, so identified, it is also possible to derive…

天体物理学 · 物理学 2009-11-13 Janet E. Drew , R. Greimel , M. J. Irwin , S. E. Sale

We present high-resolution near-infrared imaging obtained using adaptive optics and HST/NICMOS, and ground-based spectroscopy of the hot-spot galaxy NGC2903. Our near-infrared resolution imaging enables us to resolve the infrared hot spots…

天体物理学 · 物理学 2009-10-31 A. Alonso-Herrero , S. D. Ryder , J. H. Knapen

The Orion Nebula Cluster (ONC) is the closest site of very young ($\sim$ 1 Myrs) massive star formation. The ONC hosts more than 1600 young and X-ray bright stars with masses ranging from $\sim$ 0.1 to 35 $M_\odot$. The Chandra HETGS Orion…

We discuss five blue stellar systems in the direction of the Virgo cluster, analogous to the enigmatic object SECCO 1 (AGC 226067). These objects were identified based on their optical and UV morphology and followed up with HI observations…

We present observations of the star formation region NGC 7129 taken with the Multiband Imaging Photometer for Spitzer (MIPS). A significant population of sources, likely pre-main sequence members of the young stellar cluster, is revealed…

As part of the VLT/X-shooter science verification, we obtained the first optical medium-resolution spectrum of a previously identified bright O-type object in NGC55, an LMC-like galaxy at a distance of \sim2.0 Mpc. Based on the stellar and…

太阳与恒星天体物理 · 物理学 2013-01-17 Olga Hartoog , Hugues Sana , Alex de Koter , Lex Kaper