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相关论文: Observations of a high-mass protostar in NGC 7538S

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We present deep high angular resolution observations of the high-mass protostar NGC 7538S, which is in the center of a cold dense cloud core with a radius of 0.5 pc and a mass of ~2,000 Msun. These observations show that NGC 7538S is…

太阳与恒星天体物理 · 物理学 2015-05-18 Goran Sandell , Melvyn Wright

We report the detection of a massive rotating disk around the high-mass Class 0 candidate NGC 7538S. The disk is well-resolved with BIMA (HPBW =3.7") in 3.4 mm continuum and in H13CN J = 1 - 0. It is seen nearly edge on and has a size of ~…

天体物理学 · 物理学 2009-11-07 G. Sandell , M. Wright , J. R. Forster

Context: The nature of embedded accretion disks around forming high-mass stars is one of the missing puzzle pieces for a general understanding of the formation of the most massive and luminous stars. Methods: Using the Plateau de Bure…

太阳与恒星天体物理 · 物理学 2015-06-05 Henrik beuther , Hendrik Linz , Thomas Henning

We report on high-sensitivity and high-angular resolution archival Submillimeter Array (SMA) observations of the large ($\sim$15000 AU) putative circumstellar disk associated with the O-type protostar NGC 7538 S. Observations of the…

Context: High-mass stars have a high degree of multiplicity and most likely form via disk accretion processes. The detailed physics of the binary and disk formation are still poorly constrained. Methods: Using the VLA in its most extended…

太阳与恒星天体物理 · 物理学 2017-09-13 H. Beuther , H. Linz , Th. Henning , S. Feng , R. Teague

This paper reports 43 GHz imaging of the high-mass protostars W33A, AFGL 2591 and NGC 7538 IRS9 at 0.04'' and 0.6'' resolution. In each case, weak (~mJy), compact (~100 AU) emission is detected, which has an elongated shape (axis ratio ~3).…

天体物理学 · 物理学 2009-11-10 Floris van der Tak , Karl Menten

We present high resolution (R = 75,000-100,000) mid-infrared spectra of the high-mass embedded young star IRS 1 in the NGC 7538 star-forming region. Absorption lines from many rotational states of C2H2, 13C12CH2, CH3, CH4, NH3, HCN, HNCO,…

星系天体物理 · 物理学 2012-08-27 C. Knez , J. H. Lacy , N. J. Evans , II , E. F. van Dishoeck , M. J. Richter

We report new results based on the analysis of the SMA and CARMA observations of NGC 7538\,IRS\,1 at 1.3 and 3.4 mm with sub-arcsec resolutions. With angular resolutions $\sim$ 0\farcs7, the SMA and CARMA observations show that the…

太阳与恒星天体物理 · 物理学 2019-08-19 Lei Zhu , Jun-Hui Zhao , Melvyn Wright , Göran Sandell , Hui Shi , Yue-Fang Wu , Crystal Brogan , Stuartt Corder

We present deep and high-resolution (FWHM ~ 0.4 arcsec) near-infrared (NIR) imaging observations of the NGC 7538 IRS 1-3 region (in JHK bands), and IRS 9 region (in HK bands) using the 8.2m Subaru telescope. The NIR analysis is complemented…

星系天体物理 · 物理学 2015-06-22 K. K. Mallick , D. K. Ojha , M. Tamura , A. K. Pandey , S. Dib , S. K. Ghosh , K. Sunada , I. Zinchenko , L. Pirogov , M. Tsujimoto

Context: NGC 7538 IRS 1-3 is a high-mass star-forming cluster with several detected dust cores, infrared sources, (ultra)compact H$_{\rm II}$ regions, molecular outflows, and masers. In such a complex environment, important interactions and…

太阳与恒星天体物理 · 物理学 2015-06-19 Pau Frau , Josep M Girart , Qizhou Zhang , Ramprasad Rao

New high resolution observations of HCO+ J=1-0, H13CN J=1-0, SO 2,2 - 1,1, and continuum with BIMA at 3.4 mm show that the NGC7538 - IRS9 cloud core is a site of active ongoing star formation. Our observations reveal at least three young…

天体物理学 · 物理学 2009-11-10 G. Sandell , W. M. Goss , M. Wright

We have obtained high resolution mid-infrared images of the high mass protostar NGC 7538 IRS 1 using Michelle on Gemini North and find that the circumstellar dust associated with this source is extended on both large and small scales. The…

天体物理学 · 物理学 2009-11-13 James M. De Buizer , Vincent Minier

We present maps of the 850 micron and 450 micron continuum emission seen towards a sample of 68 high-mass protostellar candidates with luminosities ranging from 10^2.5 to 10^5 solar luminosity. Most of these candidate high-mass stars are in…

天体物理学 · 物理学 2009-11-10 S. J. Williams , G. A. Fuller , T. K. Sridharan

We present the first overview of the Herschel observations of the nearby high-mass star-forming region NGC 7538, taken as part of the Herschel imaging study of OB Young Stellar objects (HOBYS) Key Programme. These PACS and SPIRE maps cover…

We present the results of millimeter and centimeter continuum observations, made with the IRAM 30m telescope and the VLA, toward a sample of 11 luminous IRAS sources classified as high-mass protostellar object candidates. We find 1.2 mm…

天体物理学 · 物理学 2009-11-13 Á. Sánchez-Monge , A. Palau , R. Estalella , M. T. Beltrán , J. M. Girart

We present a Submillimeter Array study in the 1.3 mm waveband of the NGC 7538 IRS 1--3 massive star-forming region. The brightest core in the mm continuum map, MM1, harbors the IRS 1 young O star. The core has a gas temperature of about 245…

星系天体物理 · 物理学 2015-05-20 Keping Qiu , Qizhou Zhang , Karl M. Menten

We present dust polarization and CO molecular line images of NGC 7538 IRS1. We combined data from the SMA, CARMA and JCMT telescopes to make images with 2.5 arcsec resolution at 230 and 345 GHz. The images show a remarkable spiral pattern…

星系天体物理 · 物理学 2015-06-23 M. C. H. Wright , Charles Hull , Thushara Pillai , Jun-Hui Zhao , Goran Sandell

We present submillimeter continuum maps at 450 and 850 microns of a 12 x 8 arcminute region of the NGC 7538 high-mass star-forming region, made using the Submillimeter Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell…

天体物理学 · 物理学 2009-11-10 M. A. Reid , C. D. Wilson

We present high spatial resolution Submillimeter Array observations and supplementary single-dish photometry of the molecular gas and dust around IRAS 04158+2805, a young source with spectral type M5-M6 in the Taurus star-forming region. A…

天体物理学 · 物理学 2009-11-13 Sean M. Andrews , Michael C. Liu , Jonathan P. Williams , K. N. Allers

NGC 7538 IRS1 is a high-mass (approx. 30 M_sun) protostar with a CO outflow, an associated UCHII region, and a linear methanol maser structure, which might trace a Keplerian-rotating circumstellar disk. The directions of the various…

天体物理学 · 物理学 2009-11-11 S. Kraus , Y. Balega , M. Elitzur , K. -H. Hofmann , Th. Preibisch , A. Rosen , D. Schertl , G. Weigelt , E. T. Young
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