A ^{12}CO (J=1 → 0) study towards the star forming regions RCW 121 and RCW 122

Details A ^{12}CO (J=1 → 0) study towards the star forming regions RCW 121 and RCW 122 A ^{12}CO (J=1 → 0) study towards the star forming regions RCW 121 and RCW 122

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33..161d&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Astronomy and Astrophysics

Astronomy

Hii Regions, Ism: Jets And Outflows, Stars: Pre-Main Sequence, Stars: Mass Loss

Scientific paper

Using NANTEN ^{12} CO (J=1 → 0) observations (HPBW = 2'.7), we found a molecular cloud associated with the star forming regions RCW 121 and RCW 122. Kinematical properties, large scale distribution, and physical parameters were determined. Both RCW 121 and RCW 122, have very strong IR counterparts. New radiocontinuum fluxes determinations indicate that RCW 121 and RCW 122 are thermal in nature.

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