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We present a study of molecular outflows using high-resolution mapping of the CO (1-0) line emission toward eight relatively nearby 6.7 GHz methanol masers, which are associated with massive star forming regions. Outflows were detected in…

天体物理学 · 物理学 2008-11-26 Y. Xu , Z. -Q. Shen , J. Yang , X. W. Zheng , A. Miyazaki , K. Sunada , H. J. Ma , J. J. Li , J. X. Sun , C. C. Pei

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 present the analysis of two outflows (S1 at --5500 km s$^{-1}$ and S2 at --9700 km s$^{-1}$) seen in recent HST/COS observations of quasar SDSS J0755+2306 (z = 0.854). The outflows are detected as absorption troughs from both…

星系天体物理 · 物理学 2020-03-25 Xinfeng Xu , Nahum Arav , Timothy Miller , Gerard A. Kriss , Rachel Plesha

The fast outflow emerging from a region associated with massive star formation in the Orion Molecular Cloud 1 (OMC-1), located behind the Orion Nebula, appears to have been set in motion by an explosive event. Here we study the structure…

星系天体物理 · 物理学 2012-03-15 H. D. Nissen , N. J. Cunningham , M. Gustafsson , J. Bally , J. -L. Lemaire , C. Favre , D. Field

Using the Caltech Submillimeter Observatory 10.4-meter telescope, we performed sensitive mapping observations of 12CO J=7-6 emission at 807 GHz towards Orion IRc2. The image has an angular resolution of 10", which is the highest angular…

星系天体物理 · 物理学 2015-05-13 Ray S. Furuya , Hiroko Shinnaga

We present new SMA and PdBI observations of the intermediate-mass object IRAS 22198+6336 in the millimeter continuum and in several molecular line transitions. The millimeter continuum emission reveals a strong and compact source with a…

We present sub-arcsecond resolution HCN (4-3) and CO (3-2) observations made with the Submillimeter Array (SMA), toward an extremely young intermediate-mass protostellar core, MMS 6-main, located in the Orion Molecular Cloud 3 region…

星系天体物理 · 物理学 2015-06-03 Satoko Takahashi , Paul Ho

We present observations of continuum and molecular lines towards the protostar candidates IRAS 21307+5049 and IRAS 22172+5549. Single-dish maps in the 12CO(2--1), C18O(2--1), HCO+(1--0) lines and sub-mm continuum are compared with…

天体物理学 · 物理学 2009-11-10 F. Fontani , R. Cesaroni , L. Testi , S. Molinari , Q. Zhang , J. Brand , C. M. Walmsley

We examine an Infrared Dark Cloud (IRDC) at high spatial resolution as a means to study rotation, outflow, and infall at the onset of massive star formation. Submillimeter Array observations combined with IRAM 30 meter data in 12CO(2--1)…

太阳与恒星天体物理 · 物理学 2015-05-13 C. Fallscheer , H. Beuther , Q. Zhang , E. Keto , T. K. Sridharan

The red MSX source G034.5964-01.0292 (MSXG34), catalogued as a massive YSO, was observed in molecular lines with the aim of discover and study molecular outflows. We mapped a region of 3'x3' centered at MSXG34 using the Atacama…

星系天体物理 · 物理学 2014-09-05 S. Paron , M. E. Ortega , A. Petriella , M. Rubio

The protostar IRAS 15398-3359 is associated with a bipolar molecular outflow ejected in an nearly northeast-southwest (NE-SW) direction which has been extensively studied. It has been suggested previous episodic accretion events by this…

太阳与恒星天体物理 · 物理学 2024-06-12 E. Guzmán Ccolque , M. Fernández López , M. M. Vazzano , I. de Gregorio , A. Plunkett , A. Santamaría-Miranda

The Cepheus E outflow has been studied in the mid and far infrared using the ISO CAM and LWS instruments, and at millimetric wavelengths using OVRO. In the near and mid-IR, its morphology is similar to that expected for a jet driven…

天体物理学 · 物理学 2009-11-06 A. Moro-Martin , A. Noriega-Crespo , S. Molinari , L. Testi , J. Cernicharo , A. Sargent

Using the Very Long Baseline Array and the European VLBI Network, we have observed 22.2 GHz H_2O and 1612 MHz OH masers in the "water fountain" source IRAS 18460-0151. The H_2O maser spectrum has a very wide line-of-sight velocity range…

太阳与恒星天体物理 · 物理学 2015-06-16 Hiroshi Imai , Shuji Deguchi , Jun-ichi Nakashima , Sun Kwok , Philip J. Diamond

We present and discuss \emph{Spitzer} and near-infrared H$_{2}$ observations of a new bi-polar protostellar outflow in the Rosette Molecular Cloud. The outflow is seen in all four IRAC bands and partially as diffuse emission in the MIPS 24…

太阳与恒星天体物理 · 物理学 2015-05-18 Jason E. Ybarra , Elizabeth A. Lada , Zoltan Balog , Scott W Fleming , Randy L. Phelps

We report ALMA long-baseline observations of Orion Source I (SrcI) with resolution 0.03-0.06" (12-24 AU) at 1.3 and 3.2 mm. We detect both continuum and spectral line emission from SrcI's disk. We also detect a central weakly resolved…

星系天体物理 · 物理学 2018-07-04 Adam Ginsburg , John Bally , Ciriaco Goddi , Richard Plambeck , Melvyn Wright

Over the past few years, chemical studies have revealed multiple structures in the vicinity of young stellar objects (YSOs). It has become evident that specific physical conditions are associated with the emission of particular molecular…

太阳与恒星天体物理 · 物理学 2024-07-03 M. Tanious , R. Le Gal , R. Neri , A. Faure , A. Gupta , C. J. Law , J. Huang , N. Cuello , J. P. Williams , F. Ménard

We report on subarcsecond observations of complex organic molecules (COMs) in the high-mass protostar IRAS20126+4104 with the Plateau de Bure Interferometer in its most extended configurations. In addition to the simple molecules SO, HNCO…

We present a millimeter wave study of a cluster of bipolar CO outflows embedded in the western end of the Circinus molecular cloud complex, G317-4, that is traced by very high optical extinction. For an assumed distance of 700 pc, the…

天体物理学 · 物理学 2014-10-13 John Bally , Bo Reipurth , Charles J. Lada , Youssef Billawala

This paper investigates small-scale structures of dense gas and dust around the low-mass protostellar binary NGC1333-IRAS2 using millimeter-wavelength aperture-synthesis observations from the OVRO and BIMA interferometers. The detected 3 mm…

天体物理学 · 物理学 2009-11-10 J. K. Jorgensen , M. R. Hogerheijde , E. F. van Dishoeck , G. A. Blake , F. L. Schoeier