Results 51 to 60 of about 14,604 (166)
To reveal the origin of the mini-starbursts in the Milky Way, we carried out large-scale CO observations toward the RCW 106 giant molecular cloud (GMC) complex using the NANTEN2 4 m radio telescope operated by Nagoya University.
Mikito Kohno +15 more
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High altitude molecular clouds [PDF]
A population of molecular clouds with a significantly greater scale height than that of Giant Molecular Clouds has been identified by examining maps of the latitude distribution of the $^{12}CO(1-0)$ emission in the first quadrant of the Galaxy. These clouds are found by identifying emission more than 2.6 times the scale-height away from the galactic ...
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Cloud-to-cloud Velocity Dispersions Across a Local Arm Segment
Using a large sample of 9617 molecular clouds (MCs) from the Milky Way Imaging Scroll Painting survey, we mainly measure one-dimensional cloud-to-cloud velocity dispersions across a 450 deg ^2 segment of the Local Arm in the Galactic second quadrant.
Lixia Yuan, Ji Yang
doaj +1 more source
In the present work, we suggest a new approach for studying the equilibrium states of an hydrodynamic isothermal turbulent self-gravitating system as a statistical model for a molecular cloud. The main hypothesis is that the local turbulent motion of the
Sava Donkov +2 more
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On the Flux–Intensity Relation of Molecular Clouds
In this work, we report a study on the relationship between flux and intensity for molecular clouds. Our analysis is established on high-quality CO images from the Milky Way Imaging Scroll Painting project.
Qing-Zeng Yan +9 more
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Herschel/HIFI observations of molecular lines toward G10.47+0.03
We present a spectral line analysis of the hot molecular core G10.47 + 0.03 (hereafter, G10). Our aim is to determine molecular abundances and excitation conditions across a wide spectral range inaccessible to ground-based observatories.
Indrajit Mondal +12 more
doaj +1 more source
Quantification of the Role of Chemical Desorption in Molecular Clouds. [PDF]
Fredon A, Radchenko AK, Cuppen HM.
europepmc +1 more source
Supernova remnants in molecular clouds [PDF]
31 pages, 4 figures, revised, in press, ApJ, Feb.
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Examining Turbulence in Galactic Molecular Clouds. I. A Statistical Analysis of Velocity Structures
We present a systematic analysis of the velocity structure functions (VSFs) of 167 molecular clouds with angular sizes greater than ~176 arcmin ^2 in three sectors of the Galactic midplane.
Yuehui Ma +16 more
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Star Formation in Molecular Clouds [PDF]
We examine how star formation occurs in the Galaxy and come to the following conclusions. (1) The distribution of newly-born stars in the Galaxy depends on the origin of giant-molecular-cloud complexes. For individual complexes, we favor the mechanism of Parker's instability behind galactic shocks.
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