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The largest molecular complexes in the first Galactic quadrant

Published online by Cambridge University Press:  04 August 2017

T. M. Dame ,
B. G. Elmegreen ,
R. S. Cohen  and
P. Thaddeus
T. M. Dame
Affiliation:
Goddard Institute for Space Studies and Columbia University New York City
B. G. Elmegreen
Affiliation:
Goddard Institute for Space Studies and Columbia University New York City
R. S. Cohen
Affiliation:
Goddard Institute for Space Studies and Columbia University New York City
P. Thaddeus
Affiliation:
Goddard Institute for Space Studies and Columbia University New York City

Extract

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The CO emission within a few kiloparsecs of the Sun is dominated by a small number of very large molecular complexes, including those associated with the Orion Nebula (Thaddeus 1982), M16 and M17 (Elmegreen, Lada, and Dickinson 1979), and NGC7538 (Cohen et al. 1980). These complexes have masses from several 105 to 106 M⊙ and are generally very well-defined objects. They are also well endowed with HII regions, stellar clusters and associations, masers, and other Population-I objects whose distances can be measured. The complexes are thus valuable probes of the large-scale structure of the Galaxy.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 303 - 304
Copyright
Copyright © Reidel 1985 

References

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