中文
相关论文

相关论文: Sequential star formation in a cometary globule (B…

200 篇论文

We have made an extensive survey of emission-line stars in the IC 1396 HII region to investigate the low-mass population of pre-main sequence (PMS) stars. A total of 639 H-alpha emission-line stars were detected in an area of 4.2 deg^2 and…

太阳与恒星天体物理 · 物理学 2015-06-03 M. Nakano , K. Sugitani , M. Watanabe , N. Fukuda , D. Ishihara , M. Ueno

We have investigated the young stellar population in and around SFO 38, one of the massive globules located in the northern part of the Galactic HII region IC 1396, using the Spitzer IRAC and MIPS observations (3.6 to 24 micron) and…

星系天体物理 · 物理学 2015-05-18 Rumpa Choudhury , Bhaswati Mookerjea , H. C. Bhatt

Context. The formation and early evolution of high- and intermediate-mass stars towards the main sequence involves the interplay of stars in a clustered and highly complex environment. To obtain a full census of this interaction, the…

太阳与恒星天体物理 · 物理学 2015-05-28 K. M. Maaskant , A. Bik , L. B. F. M. Waters , L. Kaper , Th. Henning , E. Puga , M. Horrobin , J. Kainulainen

We present a large-scale study of the IC1396 region using new deep NIR and optical images, complemented by 2MASS data. For ten globules in IC1396 we determine (H-K, J-H) colour-colour diagrams and identify the young stellar population. Five…

天体物理学 · 物理学 2009-11-10 Dirk Froebrich , Alexander Scholz , Jochen Eislöffel , Gareth C. Murphy

We present in this paper a comprehensive study of the H II region IC 1396 and its star formation activity, in which multi-wavelength data ranging from the optical to the near- and far-infrared were employed. The surface density distribution…

太阳与恒星天体物理 · 物理学 2015-06-12 Ya Fang Huang , Jin Zeng Li

We present VLT/SINFONI integral field spectroscopy of RCW 34 along with Spitzer/IRAC photometry of the surroundings. RCW 34 consists of three different regions. A large bubble has been detected on the IRAC images in which a cluster of…

We have made a new survey of emission-line stars in the W5E HII region to investigate the population of PMS stars near the OB stars by using the Wide Field Grism Spectrograph 2 (WFGS2). A total of 139 H-alpha emission stars were detected…

天体物理学 · 物理学 2015-05-13 Makoto Nakano , Koji Sugitani , Takahiro Niwa , Yoichi Itoh , Makoto Watanabe

We present results from a study of two luminous IRAS sources thought to be young massive star-forming regions and which have no previously detected radio continuum emission: IRAS 15596-5301 and IRAS 16272-4837. Our study incorporates…

天体物理学 · 物理学 2007-05-23 K. J. Brooks , G. Garay , D. Mardones , R. P. Norris , M. G. Burton

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…

星系天体物理 · 物理学 2020-06-29 Mauricio Tapia , Paolo Persi , Miguel Roth , Davide Elia

The IC 1396N cometary globule within the large nearby HII region IC 1396 has been observed with the ACIS detector on board the Chandra X-ray Observatory. We detect 117 X-ray sources, of which ~50-60 are likely members of the young open…

天体物理学 · 物理学 2008-11-26 Konstantin V. Getman , Eric D. Feigelson , Gordon Garmire , Patrick Broos , Junfeng Wang

We present a multi-wavelength study to analyse the star formation process associated with the mid-infrared bubble CN 148 (H II region G10.3-0.1), which harbors an O5V-O6V star. The arc-shaped distribution of molecular CO(2-1) emission, the…

星系天体物理 · 物理学 2015-06-23 L. K. Dewangan , D. K. Ojha , J. M. C. Grave , K. K. Mallick

BVRIJHK photometry, Spitzer-GLIMPSE photometry and HK band spectroscopy were used to study the stellar content of IRAS 19343+2026, a (proto)star/cluster candidate, located close to the Galactic plane. The data suggest that IRAS 19343+2026…

星系天体物理 · 物理学 2015-05-19 D. K. Ojha , M. S. N. Kumar , C. J. Davis , J. M. C. Grave

We report Radio Recombination Line (RRL) and continuum observations toward the IRAS point source 16362--4845, embedded within the Bright-Rimmed Cloud (BRC) SFO 79, a small molecular cloud lying at the edge of the HII region RCW 108. High…

天体物理学 · 物理学 2009-11-10 J. S. Urquhart , M. A. Thompson , L. K. Morgan , Glenn J. White

We have observed the IC1396W globule in a narrow band filter centred on the 1-0 S(1) line of molecular hydrogen and in the J, H, K' broad-band filters. Three molecular hydrogen outflows could be identified by means of H2 emission. The…

天体物理学 · 物理学 2009-11-07 D. Froebrich , A. Scholz

Bright-rimmed clouds (BRCs) found in H II regions are probable sites of triggered star formation due to compression by ionization/shock fronts, and it is hypothesized that star formation proceeds from the exciting star(s) side outward of…

天体物理学 · 物理学 2015-06-24 Katsuo Ogura , Neelam Chauhan , Anil K. Pandey , Bhuwan C. Bhatt , Devendra Ojha , Yoichi Itoh

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 report sensitive ATCA radio-continuum observations toward IRAS 15596-5301 and 16272-4837, two luminous objects (> 2x10^4 Lsun) thought to represent massive star-forming regions in early stages of evolution (due to previously undetected…

天体物理学 · 物理学 2011-03-10 Guido Garay , Kate Brooks , Diego Mardones , Ray P. Norris , Michael G. Burton

We investigate the young stellar population in and near the cometary globule Ori,I-2. The analysis is based on deep Nordic Optical Telescope R-band and H-alpha images, JCMT SCUBA 450 and 850 micron images combined with near-infrared 2MASS…

星系天体物理 · 物理学 2014-11-20 B. Mookerjea , G. Sandell

The intermediate- to high-mass star-forming region IRAS 20343+4129 is an excellent laboratory to study the influence of high- and intermediate-mass young stellar objects on nearby starless dense cores, and investigate for possible…

星系天体物理 · 物理学 2015-06-04 F. Fontani , Aina Palau , G. Busquet , A. Isella , R. Estalella , A. Sanchez-Monge , P. Caselli , Q. Zhang

By means of different physical mechanisms, the expansion of HII regions can promote the formation of new stars of all masses. RCW 120 is a nearby Galactic HII region where triggered star formation occurs. This region is well-studied - there…

‹ 上一页 1 2 3 10 下一页 ›