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The headlight cloud in NGC 628: An extreme giant molecular cloud in a typical galaxy disk
(EDP Sciences, 2020)
Context. Cloud-scale surveys of molecular gas reveal the link between giant molecular cloud properties and star formation across a range of galactic environments. Cloud populations in galaxy disks are considered to be ...
Constraints on free–free emission from anomalous microwave emission sources in the perseus molecular cloud
(The American Astronomical Society, 2013-06-20)
We present observations performed with the Green Bank Telescope at 1.4 and 5 GHz of three strips coincident with
the anomalous microwave emission features previously identified in the Perseus molecular cloud at 33 GHz ...
Discovery of a dense molecular cloud towards a young massive embedded star in 30 Doradus
(2009)
Context. The 30 Doradus region in the Large Magellanic Cloud is one of the most outstanding star-forming regions of the Local Group and a primary target for studying star formation in an environment of low metallicity. ...
Studying the molecular gas towards a bright rimmed cloud at the infrared dust bubble N30
(Asociación Argentina de Astronomía, 2020)
We present a study on the molecular gas towards a bright-rimmed cloud located to the north of theinfrared dust bubble N30. Using the emission from the12CO,13CO, and C18O J=3?2 line, together with infraredand radio continuum ...
The matter between the starsLa materia entre las estrellas
(Facultad de Ciencias, 2010)
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
(2008)
We have carried out submillimeter 12CO(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 high ...
Results of the SEST Key Programme: CO in the Magellanic Clouds VIII. The giant molecular complex No. 37 of the LMC
(2002)
We report observations of the CO(1!0), CO(2!1) and 13CO(1!0) line emission from the giant molecular
complex No. 37 of the Large Magellanic Cloud, made with linear resolutions between 6 and 12 pc. The observations
were ...
Rotation in molecular clouds
(1999)
We have investigated a broad range of evidence concerning rotation in molecular clouds. As a consequence, we show that trends in specific angular momentum J/M and angular velocity ? are inconsistent with certain models of ...