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We have made 12CO 2-1 and 1-0 maps of eleven molecular outflows associated with intermediate to high-mass young stellar objects (YSOs) in order to establish whether the correlations between outflow parameters and source bolometric…

Astrophysics · Physics 2009-11-07 Naomi A. Ridge , Toby J. T. Moore

We report interferometric observations of the VeLLO L1521F-IRS, in 12CO (2-1) line emission and the 1.3 mm continuum emission, using the Submillimeter Array (SMA). With the 12CO high-resolution observations, we have spatially resolved a…

Astrophysics of Galaxies · Physics 2015-06-16 Satoko Takahashi , Nagayoshi Ohashi , Tyler Bourke

Jets and outflows trace the accretion history of protostars. High-velocity molecular jets have been observed from several protostars in the early Class\,0 phase of star formation, detected with the high-density tracer SiO. Until now, no…

Low-ionization-state far-infrared (FIR) emission lines may be useful diagnostics of star-formation activity in young galaxies, and at high redshift may be detectable from the ground. In practice, however, very little is known concerning how…

Astrophysics · Physics 2009-11-10 Gaelen Marsden , Colin Borys , Scott C. Chapman , Mark Halpern , Douglas Scott

We report the first systematic survey of molecular lines (including HCO+ (1-0) and 12CO, 13CO, C18O (1-0) lines at 3 mm band) towards a new sample of 88 massive young stellar object (MYSO) candidates associated with ongoing outflows (known…

Solar and Stellar Astrophysics · Physics 2014-11-20 Xi Chen , Zhi-Qiang Shen , Jing-jing Li , Ye Xu , Jin-hua He

We present new ultraviolet (UV) observations of the luminous compact blue galaxy KISSR242, obtained with the HST-COS. We identify multiple resolved sub-arcsecond near-UV sources within the COS aperture. The far-UV spectroscopic data show…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Kevin France , Nicholas Nell , James C. Green , Claus Leitherer

We investigate the properties of star formation-driven outflows by using a large spectroscopic sample of ~160,000 local "normal" star forming galaxies, drawn from the SDSS, spanning a wide range of star formation rates and stellar masses.…

Astrophysics of Galaxies · Physics 2016-03-16 Claudia Cicone , Roberto Maiolino , Alessandro Marconi

We have undertaken the largest survey for outflows within the Galactic Plane using simultaneously observed 13CO and C18O data. 325 out of a total of 919 ATLASGAL clumps have data suitable to identify outflows, and 225 (69+-3%) of them show…

Astrophysics of Galaxies · Physics 2018-09-05 Aiyuan Yang , Mark Thompson , James Urquhart , Wenwu Tian

We present a search for CO emission in a sample of ten type-2 quasar host galaxies with redshifts of z=0.1-0.4. We detect CO(J=1-0) line emission with >=5sigma in the velocity integrated intensity maps of five sources. A sixth source shows…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 M. Krips , R. Neri , P. Cox

We present high sensitivity and high angular resolution images of the high velocity (vLSR>30kms^-1) CO emission in the J=1-0 and J=2-1 lines of the Orion KL region. These results reveal the morphology of the high-velocity CO emission at the…

Astrophysics · Physics 2007-05-23 A. Rodriguez-Franco , J. Martin-Pintado , T. L. Wilson

We present velocities of galactic outflows in seven star-forming galaxies at $z=$5-6 with stellar masses of $M_* \sim10^{10.1}\ \rm{M_\odot}$. Although it is challenging to observationally determine the outflow velocities, we overcome this…

Astrophysics of Galaxies · Physics 2019-12-18 Yuma Sugahara , Masami Ouchi , Yuichi Harikane , Nicolas Bouché , Peter D. Mitchell , Jérémy Blaizot

We have used widely spaced in time Hubble Space Telescope images to determine tangential velocities of features associated with outflows from young stars. These observations were supplemented by groundbased telescope spectroscopy and from…

Astrophysics · Physics 2009-11-13 C. R. O'Dell , W. J. Henney

In this paper, we perform an analysis of 13 outflows in the Cygnus X star-forming region. We use the James Clerk Maxwell Telescope observations of $^{13}$CO(3-2) and C$^{18}$O(3-2) molecular emission lines combined with archival…

Astrophysics of Galaxies · Physics 2021-04-26 Soumen Deb , Roland Kothes , Erik Rosolowsky

We present molecular line, H2O maser, radio continuum and near infrared maps of the bipolar outflow source AFGL5142. The high resolution of our molecular CO observations enables us to define the morphology of the large-scale bipolar outflow…

Dense atomic jets from young stars copiously emit in [FeII] IR lines, which can, therefore, be used to trace the immediate environments of embedded protostars. We want to investigate the morphology of the bright [FeII] 1.64um line in the…

Solar and Stellar Astrophysics · Physics 2014-07-02 S. Antoniucci , A. La Camera , B. Nisini , T. Giannini , D. Lorenzetti , D. Paris , E. Sani

We present the results of a high angular resolution Very Large Array (VLA) Class I 44 GHz and Class II 6.7 GHz methanol maser survey of a sample of ~20 massive young stellar object (MYSO) outflow candidates selected on the basis of extended…

Solar and Stellar Astrophysics · Physics 2009-09-28 C. J. Cyganowski , C. L. Brogan , T. R. Hunter , E. Churchwell

With the observations of the CS 5-4 line toward a sample of 24 infrared bright galaxies using HHSMT, we detected CS 5-4 emission in 14 galaxies, including 12 ULIRGs/LIRGs and 2 nearby normal galaxies. As a good dense gas tracer, which has…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Junzhi Wang , Zhiyu Zhang , Yong Shi

Galactic outflows provide important feedback effects to regulate the evolution of host galaxies. Two primary diagnostics of outflows are broad and/or blueshifted emission and absorption lines. Even though well-established methods exist to…

Using CARMA, we imaged the 87 GHz SiO v=0 J=2-1 line toward Orion-KL with 0.45 arcsec angular resolution. The maps indicate that radio source I drives a bipolar outflow into the surrounding molecular cloud along a NE--SW axis, in agreement…

Gas plays a major role in the dynamical evolution of young stellar objects. Its interaction with the dust is the key to our understanding planet formation later on in the protoplanetary disc stage. Studying the gas content is a crucial step…

Solar and Stellar Astrophysics · Physics 2016-10-19 Pablo Rivière Marichalar , Bruno Merín , Inga Kamp , Carlos Eiroa , Benjamín Montesinos
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