Observation and study of the CO molecular lines towards IRAS 05437-0001 and IRAS 05351+3549.

Details Observation and study of the CO molecular lines towards IRAS 05437-0001 and IRAS 05351+3549. Observation and study of the CO molecular lines towards IRAS 05437-0001 and IRAS 05351+3549.

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000acasn..41...28j&link_type=abstract

Acta Astron. Sin., Vol. 41, No. 1, p. 28 - 35

Astronomy and Astrophysics

Astronomy

4

Young Stellar Objects: Carbon Monoxide, Young Stellar Objects: Star Formation, Young Stellar Objects: Molecular Outflows

Scientific paper

The authors observed CO(1-0) spectral lines towards IRAS 05437-0001 and IRAS 05351+3549 as well as their adjacent areas with the 13.7 m radio telescope in Delingha, Qinghai. Both sources show intense CO emission. The CO lines exhibit conspicuous wings, suggesting molecular outflows. A 5'×5' map for each area has been constructed. The authors conclude that these sources are those of molecular outflow. It is concluded from the dynamic time scale and IR spectral type of each source that both are young stellar objects (with ages of a few 105 years).

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