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相关论文: An Optical Survey of the Partially Embedded Young …

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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…

The reflection nebula NGC 7129 has long been known to be a site of recent star formation as evidenced, e.g., by the presence of deeply embedded protostars and HH objects. However, studies of the stellar population produced in the star…

太阳与恒星天体物理 · 物理学 2015-05-13 B. Stelzer , A. Scholz

IC 1274 is a faintly luminous nebula lying on the near surface of the Lynds 227 (L227) molecular cloud. Four luminous, early-type (B0-B5) stars are located within a spherical volume ~5' in diameter that appears to be clear of heavy…

太阳与恒星天体物理 · 物理学 2015-05-30 S. E. Dahm , G. H. Herbig , Brendan P. Bowler

The region surrounding the well-known reflection nebula, NGC 7023, illuminated by a Herbig Be star, HD 200775, located in the dark cloud L1174 is studied in this work. Based on the distances and proper motion values from Gaia DR2 of 20…

太阳与恒星天体物理 · 物理学 2020-05-04 Piyali Saha , Maheswar G. , Kamath U. S. , Lee C. W , Manoj P. , Blesson Mathew , Ekta Sharma

An analysis of the candidate embedded stellar systems in the reflection nebulae vdBH-RN26, vdBH-RN38, vdBH-RN53a, GGD20, ESO95-RN18 and NGC6595 is presented. Optical spectroscopic data from CASLEO (Argentina) in conjunction with near…

天体物理学 · 物理学 2009-11-10 J. B. Soares , E. Bica , A. V. Ahumada , J. J. Claria

We present the analysis of seven band (1.2 to 8 micron) ground and space-based imaging of the NGC 7129 young stellar cluster from FLAMINGOS on MMT, 2MASS, and the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. An analysis of…

天体物理学 · 物理学 2009-11-10 R. A. Gutermuth , S. T. Megeath , J. Muzerolle , L. E. Allen , J. L. Pipher , P. C. Myers , G. G. Fazio

We examine star clusters in the irregular, starburst galaxy NGC 1569 from HST images. In addition to the two known super star clusters, we identify 45 other clusters that are compact but resolved. Integrated UVI colors of the clusters span…

天体物理学 · 物理学 2009-10-31 D. A. Hunter , R. W. O'Connell , J. S. Gallagher , T. A. Smecker-Hane

We present an analysis of K-band stellar distributions for the young stellar clusters GGD 12-15, IRAS 20050+2720, and NGC 7129. We find that the two deeply embedded clusters, GGD 12-15 and IRAS 20050+2720, are not azimuthally symmetric and…

天体物理学 · 物理学 2009-11-10 R. A. Gutermuth , S. T. Megeath , J. L. Pipher , J. P. Williams , L. E. Allen , P. C. Myers , S. N. Raines

We investigate the star formation occurring in a region well below the Galactic plane towards the optical reflection nebula ESO 368-8 (IRAS 07383-3325). We confirm the presence of a small young stellar cluster (or aggregate of tens of YSOs)…

星系天体物理 · 物理学 2015-05-14 Pedro M. Palmeirim , Joao L. Yun

Infrared images of the dark cloud core B59 were obtained with the Spitzer Space Telescope as part of the "Cores to Disks" Legacy Science project. Photometry from 3.6-70 microns indicates at least 20 candidate low-mass young stars near the…

Star formation in starbursts appears to be biased toward compact clusters, with up to 20% of all stars formed in them. Observations with HST show that many of these clusters have luminosities (-9 > Mv > -16), UBVI colors, and half-light…

天体物理学 · 物理学 2007-05-23 Francois Schweizer

Recent high-resolution observations with the Hubble Space Telescope (HST) reveal that star clusters of extraordinary luminosity and compactness are commonly found in a variety of starburst systems. There has been much speculation that these…

天体物理学 · 物理学 2009-10-28 Luis C. Ho , Alexei V. Filippenko

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…

天体物理学 · 物理学 2008-08-29 S. E. Dahm

We present results of a sensitive 76 ksec Chandra observation of the young stellar cluster in NGC 2024 (d = 415 pc) in the Orion B giant molecular cloud. Previous infrared observations have shown that this remarkable cluster contains…

天体物理学 · 物理学 2009-11-10 S. Skinner , M. Gagne , E. Belzer

The dust cloud TGU H645 P2 and embedded in it young open cluster NGC 7129 are investigated using the results of medium-band photometry of 159 stars in the Vilnius seven-colour system down to V = 18.8 mag. The photometric data were used to…

UV-to-visual spectra of eight young star clusters in the merger remnant and protoelliptical galaxy NGC 7252, obtained with the Blanco 4-m telescope on Cerro Tololo, are presented. These clusters lie at projected distances of 3-15 kpc from…

天体物理学 · 物理学 2009-10-30 Francois Schweizer , Patrick Seitzer

We present the results of the first sensitive L band (3.4 micron) imaging study of the nearby young embedded cluster NGC 2024. Two separate surveys of the cluster were acquired in order to obtain a census of the circumstellar disk fraction…

天体物理学 · 物理学 2009-10-31 Karl E. Haisch , Elizabeth A. Lada , Charles J. Lada

We investigate the star cluster system in the starburst galaxy NGC 7673 using archival Hubble Space Telescope WFPC2 broad-band images. For the first time we are able to examine the internal structures of the prominent optical clumps in this…

天体物理学 · 物理学 2009-11-07 Nicole Homeier , John S. Gallagher , Anna Pasquali

We report on results of a 96.7 ks Chandra observation of one of the youngest, most embedded and massive young stellar clusters studied in X-rays - RCW 38. We detect 460 sources in the field of which 360 are confirmed to be associated with…

天体物理学 · 物理学 2008-11-26 Scott J. Wolk , Bradley D. Spitzbart , Tyler L. Bourke , Joao Alves

We present new Spitzer photometry of the Eagle Nebula (M16, containing the optical cluster NGC 6611) combined with near-infrared photometry from 2MASS. We use dust radiative transfer models, mid-infrared and near-infrared color-color…

天体物理学 · 物理学 2009-06-23 R. Indebetouw , T. R. Robitaille , B. A. Whitney , E. Churchwell , B. Babler , M. Meade , C. Watson , M. Wolfire
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