CO(3-2),CO(2-1) and CO(1-0) observations toward the Galactic bubbles N54, N73, N74, N82 and N130

Details CO(3-2),CO(2-1) and CO(1-0) observations toward the Galactic bubbles N54, N73, N74, N82 and N130 CO(3-2),CO(2-1) and CO(1-0) observations toward the Galactic bubbles N54, N73, N74, N82 and N130

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..280p.391z&link_type=abstract

The Molecular Universe, Posters from the proceedings of the 280th Symposium of the International Astronomical Union held in Tole

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the CO(3-2), CO(2-1) and CO(1-0) observation results toward 5 bubbles, N54, N73, N74, N82 and N130. We studied the morphologies of the CO clouds associated with these bubbles and intensity ratio between CO(3-2) and CO(2-1) so as to know if there exist interaction between the bubble and ambient clouds. Combined with infrared and mm data, we found evidence for triggered star formation in several bubbles.

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