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相关论文: The young stellar population in M17 revealed by Ch…

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We present the second installment of the Massive Star-forming Regions (MSFRs) Omnibus X-ray Catalog (MOXC2), a compilation of X-ray point sources detected in Chandra/ACIS observations of 16 Galactic MSFRs and surrounding fields. MOXC2…

We report the discovery of a young massive stellar cluster embedded in an extended HII region, invisible at optical wavelengths where the extinction is $A_V \approx 28$ magnitudes, associated with the IRAS source 16177-5018. $J, H$ and…

天体物理学 · 物理学 2009-11-10 Alexandre Roman-Lopes , Zulema Abraham , Jacques Raymond Daniel Lepine

Young massive (M >10^4 Msun) stellar clusters are a good laboratory to study the evolution of massive stars. Only a dozen of such clusters are known in the Galaxy. Here we report about a new young massive stellar cluster in the Milky Way.…

Cygnus OB2 is the nearest example of a massive star forming region, containing over 50 O-type stars and hundreds of B-type stars. We have analyzed two Chandra pointings in Cyg OB2, detecting ~1700 X-ray sources, of which ~1450 are thought…

太阳与恒星天体物理 · 物理学 2015-05-27 Nicholas J. Wright , Jeremy J. Drake , Janet E. Drew , Jorick S. Vink

NGC6231 is a massive young star cluster, near the center of the Sco OB1 association. While its OB members are well studied, its low-mass population has received little attention. We present high-spatial resolution Chandra ACIS-I X-ray data,…

太阳与恒星天体物理 · 物理学 2016-12-07 F. Damiani , G. Micela , S. Sciortino

Aims. Young, massive stars have been found at projected distances R < 0.5 pc from supermassive black hole, Sgr A* at the center of our Galay. In recent years, increasing evidence has been found for the presence of young, massive stars also…

星系天体物理 · 物理学 2015-06-11 Shogo Nishiyama , Rainer Schödel

In this paper we present the source list for 3 Chandra observations of the Local Group galaxy M33. The observations are centered on the nucleus and on the star forming region NGC 604. We detect a total of 261 sources in an area of \~0.2…

天体物理学 · 物理学 2009-11-11 H. -J. Grimm , J. McDowell , A. Zezas , D. -W. Kim , G. Fabbiano

A 40 ks \emph{Chandra} ACIS-S observation of the dynamically young cluster A1367 yields new insights on X-ray emission from cluster member galaxies. We detect 59 point-like sources in the ACIS field, of which 8 are identified with known…

天体物理学 · 物理学 2009-11-07 M. Sun , S. S. Murray

We present 23 candidate X-ray binaries with luminosities down to 1.8x10^36 erg/s, in the nearby starburst galaxy NGC 4449, from observations totaling 105 ksec taken with the ACIS-S instrument on the Chandra Space Telescope. We determine…

宇宙学与河外天体物理 · 物理学 2015-05-30 Blagoy Rangelov , Andrea H. Prestwich , Rupali Chandar

We present results from an optical photometric and spectroscopic survey of the young stellar population in L1641, the low-density star-forming region of the Orion A cloud south of the Orion Nebula Cluster (ONC). Our goal is to determine…

太阳与恒星天体物理 · 物理学 2015-06-04 Wen-Hsin Hsu , Lee Hartmann , Lori Allen , Jesus Hernandez , S. T. Megeath , Gregory Mosby , John J. Tobin , Catherine Espaillat

The current census of, and stellar population in, massive Galactic star clusters is reviewed. In particular, we concentrate on a recent survey of obscured Galactic Giant H II (GHII) regions and the associated stellar clusters embedded in…

天体物理学 · 物理学 2007-05-23 Robert D. Blum , Peter S. Conti , Augusto Damineli , Elysandra Figueredo

We present a detailed investigation of X-ray source contents of eight young open clusters with ages between 4 to 46 Myr using archival X-ray data from XMM-Newton. The probable cluster memberships of the X-ray sources have been established…

太阳与恒星天体物理 · 物理学 2015-06-17 Himali Bhatt , J. C. Pandey , K. P. Singh , Ram Sagar , Brijesh Kumar

We present an analytical study of a large sample of ~109 young stellar objects in the X-ray. Our objects were detected in X-ray independent of age. Unexpectedly, the X-ray energy is somewhat correlated with the ages. It decreases with time…

太阳与恒星天体物理 · 物理学 2015-03-17 M. Hamidouche , M. Jacobson , L. W. Looney

We present Chandra X-ray data of the NGC 1333 embedded cluster, combining these data with existing Chandra data, Sptizer photometry and ground based spectroscopy of both the NGC 1333 & Serpens North clusters to perform a detailed study of…

太阳与恒星天体物理 · 物理学 2015-05-19 E. Winston , S. T. Megeath , S. Wolk , B. Spitzbart , R. Gutermuth , L. E. Allen , J. Hernandez , K. Covey , J. Muzerolle , J. L. Hora , P. C. Myers , G. G. Fazio

Aims: The objective of this study is to determine the general X-ray properties of the young stars in the external regions of the sigma Orionis cluster (tau ~ 3 Ma, d ~ 385 pc) and yield constraints on the X-ray emission of brown dwarfs.…

天体物理学 · 物理学 2009-11-13 J. Lopez-Santiago , J. A. Caballero

We have been monitoring M31 with HRC and ACIS onboard \chandra regularly in the past two years. By combining eight \chandra ACIS-I observations taken between 1999 to 2001, we have identified 204 X-ray sources within the central $\sim…

天体物理学 · 物理学 2007-05-23 A. K. H. Kong , M. R. Garcia , F. A. Primini , R. Di Stefano , S. S. Murray

In this first of two companion papers on the Orion Nebula Cluster (ONC), we present our analysis of a 63 Ksec Chandra HRC-I observation that yielded 742 X-ray detections within the 30'x30' field of view. To facilitate our interpretation of…

天体物理学 · 物理学 2008-11-26 E. Flaccomio , F. Damiani , G. Micela , S. Sciortino , F. R. Harnden , S. S. Murray , S. J. Wolk

We have studied the young low-mass pre-main sequence (PMS) stellar population associated with the massive star-forming region DR 21 by using archival X-ray Chandra observations and by complementing them with existing optical and IR surveys.…

星系天体物理 · 物理学 2015-06-17 V. M. Rivilla , I. Jimenez-Serra , J. Martin-Pintado , J. Sanz-Forcada

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…

The clusters of young stars in massive star-forming regions show a wide range of sizes, morphologies, and numbers of stars. Their highly subclustered structures are revealed by the MYStIX project's sample of 31,754 young stars in nearby…