中文
相关论文

相关论文: A VLT/NACO Study of Star Formation in the Massive …

200 篇论文

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

RCW~38 is a uniquely young ($<$1 Myr), embedded ($A_V \sim 10$) stellar cluster surrounding a pair of early O stars ($\sim$O5.5) and is one of the few regions within 2 kpc other than Orion to contain over 1000 members. X-ray and deep…

天体物理学 · 物理学 2008-08-26 Scott J. Wolk , Tyler L. Bourke , Miquela Vigil

We present a study of the structure of the high mass star-forming region RCW~38 and the spatial distribution of its young stellar population. Spitzer IRAC photometry 3-8um are combined with 2MASS near-IR data to identify young stellar…

太阳与恒星天体物理 · 物理学 2015-05-30 Elaine Winston , Scott J. Wolk , Tyler Bourke , S. Thomas Megeath , Robert Gutermuth , Brad Spitzbart

We present near-infrared imaging and spectroscopic high spatial resolution observations of the SMC region N88 containing the bright, excited, extincted and compact H II region N88A of size ~ 1 pc. To investigate its stellar content and…

宇宙学与河外天体物理 · 物理学 2015-05-14 G. Testor , J. L. Lemaire , M. Heydari-Malayeri , L. E. Kristensen , S. Diana , D. Field

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 report on the results of an approximately 90 ks Chandra observation of a complex region that hosts multiple sites of recent and active star formation in ARA OB1a. The field is centered on the embedded cluster RCW 108-IR and includes and…

We describe the results of two near infrared (K-band) imaging surveys and a three color (JHK) survey of the vicinity of NGC 7538. The limiting magnitudes are K ~ 16.5 and K ~ 17.5 mag for the K-band surveys and K ~ 15 mag for the JHK…

天体物理学 · 物理学 2009-11-10 Z. Balog , S. J. Kenyon , E. A. Lada , M. Barsony , J. Vinko , A. Gaspar

We have obtained high resolution (R = 10,000) K-band spectra of candidate young massive stars deeply embedded in (ultra-) compact HII regions (UCHIIs). In these clusters, three types of objects are identified. The first type (38 objects)…

天体物理学 · 物理学 2009-11-11 A. Bik , L. Kaper , M. M. Hanson , M. Smits

We present a JHKL survey of the massive star forming region RCW 57 (NGC 3576) based on L-band data at 3.5 micron taken with SPIREX (South Pole Infrared Explorer), and 2MASS JHK data at 1.25-2.2 micron. This is the second of two papers, the…

天体物理学 · 物理学 2009-11-11 M. Maercker , M. G. Burton , C. M. Wright

We analyze the embedded stellar content in the vicinity of the W3/W4/W5 HII regions using the FCRAO Outer Galaxy 12CO(J=1-0) Survey, the IRAS Point Source Catalog, published radio continuum surveys, and new near-infrared and molecular line…

天体物理学 · 物理学 2009-10-31 John M. Carpenter , Mark H. Heyer , Ronald L. Snell

We present Spitzer, NIR and millimeter observations of the massive star forming regions W5-east, S235, S252, S254-S258 and NGC7538. Spitzer data is combined with near-IR observations to identify and classify the young population while 12CO…

太阳与恒星天体物理 · 物理学 2015-06-19 L. Chavarria , L. Allen , C. Brunt , J. L. Hora , A. Muench , G. Fazio

Studies of star formation rely heavily on observations in the near-infrared, but they typically need information from other wavelengths for interpretation. We show that we can infer distances and estimate the membership of young stellar…

星系天体物理 · 物理学 2022-06-08 Joana Ascenso

We present deep 3.8 micron observations of the Trapezium cluster in Orion obtained with the ESO VLT. We use these data to search for infrared excess emission and evidence for protoplanetary disks associated with the faint, substellar…

天体物理学 · 物理学 2009-11-10 C. J. Lada , A. A. Muench , E. A. Lada , J. F. Alves

We report NIR broad and narrow band photometric observations in the direction of the IRAS17149-3916 source that reveal the presence of a young cluster of massive stars embedded in an HII region coincident with RCW121. These observations,…

天体物理学 · 物理学 2008-11-26 Alexandre Roman-Lopes , Zulema Abraham

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

We present the first results from a 124 night J, H, K near-infrared monitoring campaign of the dark cloud L 1003 in Cygnus OB7, an active star-forming region. Using 3 seasons of UKIRT observations spanning 1.5 years, we obtained…

太阳与恒星天体物理 · 物理学 2015-06-05 Thomas S. Rice , Scott J. Wolk , Colin Aspin

We report the results of a sensitive near-infrared JHKL imaging survey of the Trapezium cluster in Orion. We use the JHKL colors to obtain a census of infrared excess stars in the cluster. Of (391) stars brighter than 12th magnitude in the…

RCW 38 is a deeply embedded young (~1 Myr), massive star cluster located at a distance of 1.7 kpc. Twice as dense as the Orion Nebula Cluster, orders of magnitude denser than other nearby star forming regions, and rich in massive stars, RCW…

太阳与恒星天体物理 · 物理学 2017-08-30 Koraljka Muzic , Rainer Schoedel , Alexander Scholz , Vincent C. Geers , Ray Jayawardhana , Joana Ascenso , Lucas A. Cieza

We present near infrared (J, H, and K) photometry and moderate resolution (lambda/Deltalambda = 3000) K-band spectroscopy of the embedded stellar cluster in the giant H II region W31. Four of the brightest five cluster members are early…

天体物理学 · 物理学 2009-11-06 R. D. Blum , A. Damineli , P. S. Conti

We investigate the star formation activity in a young star forming cluster embedded at the edge of the RCW 41 HII region. As a complementary goal, we aim at demonstrating the gain provided by Wide-Field Adaptive Optics instruments to study…

太阳与恒星天体物理 · 物理学 2015-04-22 B. Neichel , M. R. Samal , H. Plana , A. Zavagno , A. Bernard , T. Fusco
‹ 上一页 1 2 3 10 下一页 ›