scholarly journals Bias‐free Measurement of Giant Molecular Cloud Properties

2006 ◽  
Vol 118 (842) ◽  
pp. 590-610 ◽  
Author(s):  
Erik Rosolowsky ◽  
Adam Leroy
2012 ◽  
Vol 8 (S292) ◽  
pp. 49-49
Author(s):  
N. Lo ◽  
M. R. Cunningham ◽  
P. A. Jones ◽  
L. Bronfman

AbstractWe present our preliminary results on the application of dendrogram statistics to the carbon monoxide PPV map of the giant molecular cloud G333. We obtain the dendrograms at various merging levels and found the clustering of branches is independent from the merging levels. The statistics of intensity distributions show gravity is possibly significant in this cloud and the gas may be sonic. Application of this method to other molecular lines data are required for further analysis of the cloud properties.


2014 ◽  
Vol 784 (1) ◽  
pp. 3 ◽  
Author(s):  
Dario Colombo ◽  
Annie Hughes ◽  
Eva Schinnerer ◽  
Sharon E. Meidt ◽  
Adam K. Leroy ◽  
...  

2011 ◽  
Vol 743 (1) ◽  
pp. 39 ◽  
Author(s):  
Alana Rivera-Ingraham ◽  
Peter G. Martin ◽  
Danae Polychroni ◽  
Toby J. T. Moore

2014 ◽  
Vol 569 ◽  
pp. A20 ◽  
Author(s):  
Maria Messineo ◽  
Karl M. Menten ◽  
Donald F. Figer ◽  
Ben Davies ◽  
J. Simon Clark ◽  
...  

2020 ◽  
Vol 899 (1) ◽  
pp. 23 ◽  
Author(s):  
K. P. Hall ◽  
Snežana Stanimirović ◽  
Min-Young Lee ◽  
Mark Wolfire ◽  
Paul Goldsmith

1980 ◽  
pp. 185-186
Author(s):  
J. W. Barrett ◽  
R. L. deZafra ◽  
D. B. Sanders ◽  
P. M. Solomon

1982 ◽  
Vol 4 (4) ◽  
pp. 434-440 ◽  
Author(s):  
J. B. Whiteoak ◽  
Robina E. Otrupcek ◽  
C. J. Rennie

The 4-m radio telescope of the CSIRO Division of Radiophysics at Epping is being used to survey the line emission associated with the 1→0 transition of CO (rest frequency 115.271 GHz) in the southern Milky Way. The programme includes mapping the CO distribution across giant molecular-cloud/HII-region complexes. As a first stage the emission has been observed towards bright southern HII regions. These results will not only serve as a basis for future extensive mapping but will also provide data which is directly comparable with observations of other molecular lines that have been made towards the HII regions.


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