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相关论文: A Survey of Extended H$_2$ Emission from Massive Y…

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We have carried out a near-infrared imaging survey of luminous young stellar outflow candidates using the United Kingdom Infrared Telescope. Observations were obtained in the broad band K (2.2 mu) and through narrow band filters at the…

太阳与恒星天体物理 · 物理学 2015-05-18 Watson P. Varricatt , Christopher J. Davis , Suzanne Ramsay , Stephen P. Todd

We analyse C$^{18}$O ($J=3-$2) data from a sample of 99 infrared-bright massive young stellar objects (MYSOs) and compact HII regions that were identified as potential molecular-outflow sources in the Red MSX source (RMS) survey. We extract…

太阳与恒星天体物理 · 物理学 2015-09-02 L. T. Maud , S. L. Lumsden , T. J. T. Moore , J. C. Mottram , J. S. Urquhart , A. Cicchini

Young stellar objects (YSOs) may undergo periods of active accretion (outbursts), during which the protostellar accretion rate is temporarily enhanced by a few orders of magnitude. Whether or not these accretion outburst YSOs possess…

Near-infrared H- and K-band spectra are presented for 247 objects, selected from the Red MSX Source (RMS) survey as potential young stellar objects (YSOs). 195 (~80%) of the targets are YSOs, of which 131 are massive YSOs (L_BOL > 5x10^3…

The luminous Young Stellar Object (YSO) IRAS 07422-2001 is studied in the infrared. We discover star forming activity in embedded clusters located in a cloud detected at mid-IR wavelengths in emission. Multiple outflows are discovered from…

太阳与恒星天体物理 · 物理学 2015-06-04 Watson P. Varricatt

The G333 giant molecular cloud contains a few star clusters and H II regions, plus a number of condensations currently forming stars. We have mapped 13 of these sources with the appearance of young stellar objects (YSOs) with the Spitzer…

星系天体物理 · 物理学 2015-05-30 Janet P. Simpson , Angela S. Cotera , Michael G. Burton , Maria Cunningham , Nadia Lo , Indra Bains

Aims: We aim to understand the star formation associated with the luminous young stellar object (YSO) IRAS 18345-0641 and to address the complications arising from unresolved multiplicity in interpreting the observations of massive…

太阳与恒星天体物理 · 物理学 2015-06-15 Watson P. Varricatt , Holly S. Thomas , Chris J. Davis , Suzanne Ramsay , Malcolm J. Currie

Massive stars form whilst they are still embedded in dense envelopes. As a result, the roles of rotation, mass loss and accretion in massive star formation are not well understood. This study evaluates the source of the Q-band, lambda=19.5…

太阳与恒星天体物理 · 物理学 2015-06-04 H. E. Wheelwright , W. J. de Wit , R. D. Oudmaijer , M. G. Hoare , S. L. Lumsden , T. Fujiyoshi , J. L. Close

We present medium-resolution (R~7000) near-infrared echelle spectroscopic data for 36 MYSOs drawn from the Red MSX Source (RMS) survey. This is the largest sample observed at this resolution at these wavelengths of MYSOs to date. The…

太阳与恒星天体物理 · 物理学 2017-09-14 R. Pomohaci , R. D. Oudmaijer , S. L. Lumsden , M. G. Hoare , I. Mendigutia

A comprehensive picture of high-mass star formation has remained elusive, in part because examples of high-mass YSOs tend to be relatively distant, deeply embedded, and confused with other emission sources. These factors have impeded…

天体物理学 · 物理学 2009-11-13 L. D. Matthews , C. Goddi , L. J. Greenhill , C. J. Chandler , M. J. Reid , E. M. L. Humphreys

Theoretical models suggest that massive stars form via disk-mediated accretion, with bipolar outflows playing a fundamental role. A recent study toward massive molecular outflows has revealed a decrease of the SiO line intensity as the…

We present mid-infrared (MIR) observations, made with the TIMMI2 camera on the ESO 3.6 m telescope, toward 14 young massive star-forming regions. All regions were imaged in the N band, and nine in the Q band, with an angular resolution of ~…

星系天体物理 · 物理学 2011-02-11 Esteban F. E. Morales , Diego Mardones , Guido Garay , Kate J. Brooks , Jaime E. Pineda

Accretion in young stellar objects (YSOs) is at least partially episodic, i.e. periods with high accretion rates ('bursts') are interspersed by quiescent phases. These bursts manifest themselves as eruptive variability. Here we present a…

太阳与恒星天体物理 · 物理学 2015-06-12 Aleks Scholz , Dirk Froebrich , Kenneth Wood

We present single pointing observations of SiO, HCO$^+$ and H$^{13}$CO$^+$ from the James Clerk Maxwell Telescope towards 23 massive star forming regions previously known to contain molecular outflows and ultracompact HII regions. We…

天体物理学 · 物理学 2019-08-19 P. D. Klaassen , C. D. Wilson

We present Spitzer IRAC images that indicate the presence of cavities cut into the dense outer envelope surrounding very young pre-main sequence stars. These young stellar objects (YSOs) characterized by an outflow represent the earliest…

天体物理学 · 物理学 2007-11-28 Jonathan P. Seale , Leslie W. Looney

We have discovered 12 new molecular hydrogen emission-line objects (MHOs) in the vicinity of the candidate massive young stellar object Mol 121, in addition to five that were previously known. H2 2.12-micron/H2 2.25-micron flux ratios…

星系天体物理 · 物理学 2015-06-12 G. Wolf-Chase , K. Arvidsson , M. Smutko , R. Sherman

M17 is one of the youngest and most massive nearby star-formation regions in the Galaxy. It features a bright H II region erupting as a blister from the side of a giant molecular cloud (GMC). Combining photometry from the Spitzer GLIMPSE…

Context: The Red MSX Source (RMS) survey has identified a large sample of candidate massive young stellar objects (MYSOs) and ultra compact (UC) HII regions from a sample of ~2000 MSX and 2MASS colour selected sources. Aims: To search for…

Jets and outflows are the first signposts of stellar birth. Emission in the H2 1-0S(1) line at 2.122 micron is a powerful tracer of shock excitation in these objects. Here we present the analysis of 2.0 x 0.8 square degrees data from the UK…

星系天体物理 · 物理学 2018-06-06 Manash R. Samal , Wen-Ping Chen , Michihiro Takami , Jessy Jose , Dirk Froebrich

We present a parsec-scale molecular hydrogen (H$_2$ 1-0 S(1) at 2.12~\micron) outflow discovered from the UKIRT Widefield Infrared Survey for H$_2$. The outflow is located in the infrared dark cloud core MSXDC G053.11+00.05 MM1 at 1.7 kpc…

星系天体物理 · 物理学 2018-08-15 Hyun-Jeong Kim , Bon-Chul Koo , Tae-Soo Pyo , Christopher J. Davis
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