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A molecular outflow revealing star formation activity in the vicinity of the HII region G034.8-0.7 and the SNR W44
(2009)
Aims. This work aims at investigating the molecular gas component in the vicinity of two young stellar object (YSO) candidates identified at the border of the HII region G034.8-0.7 that is evolving within a molecular cloud ...
A submillimeter study of the IR dust bubble s 21 and its environs
(Universidad Nacional Autonoma de Mexico, 2017)
Based on the molecular emission in the 12CO(2-1) and 13CO(2-1) lines, and on the continuum emission in the MIR and FIR towards the S 21 IR dust bubble, we analyze the physical characteristics of the gas and dust linked to ...
A view of Large Magellanic Cloud H ii regions N159, N132, and N166 through the 345-GHz window
(Oxford University Press, 2015-11)
We present results obtained towards the H II regions N159, N166, and N132 from the emission of several molecular lines in the 345 GHz window. Using Atacama Submillimetre Telescope Experiment, we mapped a 2.4 arcmin × 2.4 ...
Star forming regions linked to RCW78 and the discovery of a new IR bubble
(ESO, 2014)
Aims. With the aim of investigating the presence of molecular and dust clumps linked to two star forming regions identified in the
expanding molecular envelope of the stellar wind bubble RCW78, we analyzed the distribution ...
Chemistry of the high-mass protostellar molecular clump IRAS 16562–3959
(IOP Publishing, 2018-06)
We present molecular line observations of the high-mass molecular clump IRAS 16562-3959 taken at 3 mm using the Atacama Large Millimeter/submillimeter Array at 1.'' 17 angular resolution (0.014 pc spatial resolution). This ...
Chemistry of the High-mass Protostellar Molecular Clump IRAS 16562-3959
(Institute of Physics Publishing, 2018)
We present molecular line observations of the high-mass molecular clump IRAS
16562−3959 taken at 3 mm using the Atacama Large Millimeter/submillimeter Array (ALMA) at 1.
007 angular resolution (0.014 pc spatial resolution). ...
DISCOVERY OF A MASSIVE PROTOSTAR NEAR IRAS 18507+0121
(The American Astronomical Society, 2004-02-20)
We have observed the massive star-forming region IRAS 18507+0121 at millimeter wavelengths in 3 mm
continuum emission, H13CO+ ( J ¼ 1 0) and SiO (v ¼ 0, J ¼ 2 1) line emission, and at near-infrared (NIR)
wavelengths ...
Submillimeter observations of giant molecular clouds in the Large Magellanic Cloud: Temperature and density as determined from J=3-2 and J=1-0 transitions of CO
(UNIV CHICAGO PRESS, 2008-04)
We have carried out submillimeter (CO)-C-12(J = 3-2) observations of six giant molecular clouds (GMCs) in the Large Magellanic Cloud (LMC) with the ASTE 10 m submillimeter telescope at a spatial resolution of 5 pc and very ...