Several 1.0 continuum mapping observations were made of seven southern hemisphere h12/molecular cloud complexes with 65 arcsec resolution. The radial density distribution of the clouds with central luminosity sources was determined observationally. Strong similarities in morphology and general physical conditions were found to exist among all of the southern clouds in the sample
Regions of massive star formation have long been believed to have a profound influence on the struct...
A catalog of southern dust cloud properties is being compiled to aid in the planning and analysis of...
With the onset of the HI Parkes All-Sky Survey, a new view of the high-velocity cloud (HVC) distribu...
The property of dust in four southern H II region/molecular cloud complexes (RCW 108, RCW 57, RCW 12...
W31 is a H II region/molecular cloud complex in the galactic plane at a distance of 6 Kpc. This comp...
We present results from a 2300 arcmin^2 survey of the Orion A molecular cloud at 450 and 850 micron ...
This is the published version, also available her: http://dx.doi.org/10.1088/0004-637X/746/1/11.We p...
We present (1) new fully sampled maps of CO and (CO)-C-13 J = 2-1 emission and CO J = 3-2 emission t...
We present the results of N2H+(1–0) observations of 35 dense molecular cloud cores from the northern...
Artículo de publicación ISI.The Columbia University–Universidad de Chile CO Survey of the southern M...
Context. New-generation spectroscopic surveys of the Milky Way plane have been revealing the structu...
We have observed two rotational transitions of both CS and C17O, and the 1.2 mm continuum emission t...
We present (1) new fully sampled maps of CO and {}13{CO} J = 2-1 emission and CO J = 3-2 emission to...
Galactic CO line emission at 115 GHz was surveyed in order to study the distribution of molecular cl...
This thesis presents an observational study of molecular abundances in the dense cores of 27 promine...
Regions of massive star formation have long been believed to have a profound influence on the struct...
A catalog of southern dust cloud properties is being compiled to aid in the planning and analysis of...
With the onset of the HI Parkes All-Sky Survey, a new view of the high-velocity cloud (HVC) distribu...
The property of dust in four southern H II region/molecular cloud complexes (RCW 108, RCW 57, RCW 12...
W31 is a H II region/molecular cloud complex in the galactic plane at a distance of 6 Kpc. This comp...
We present results from a 2300 arcmin^2 survey of the Orion A molecular cloud at 450 and 850 micron ...
This is the published version, also available her: http://dx.doi.org/10.1088/0004-637X/746/1/11.We p...
We present (1) new fully sampled maps of CO and (CO)-C-13 J = 2-1 emission and CO J = 3-2 emission t...
We present the results of N2H+(1–0) observations of 35 dense molecular cloud cores from the northern...
Artículo de publicación ISI.The Columbia University–Universidad de Chile CO Survey of the southern M...
Context. New-generation spectroscopic surveys of the Milky Way plane have been revealing the structu...
We have observed two rotational transitions of both CS and C17O, and the 1.2 mm continuum emission t...
We present (1) new fully sampled maps of CO and {}13{CO} J = 2-1 emission and CO J = 3-2 emission to...
Galactic CO line emission at 115 GHz was surveyed in order to study the distribution of molecular cl...
This thesis presents an observational study of molecular abundances in the dense cores of 27 promine...
Regions of massive star formation have long been believed to have a profound influence on the struct...
A catalog of southern dust cloud properties is being compiled to aid in the planning and analysis of...
With the onset of the HI Parkes All-Sky Survey, a new view of the high-velocity cloud (HVC) distribu...