The new high-velocity molecular outflow of IRAS 19282+1814

Details The new high-velocity molecular outflow of IRAS 19282+1814 The new high-velocity molecular outflow of IRAS 19282+1814

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002acasn..43..353s&link_type=abstract

Acta Astronomica Sinica, vol.43, no.4, p. 353-358

Other

Infrared: Stars, Ism: Jets And Outflows, Stars: Formation

Scientific paper

Mapping with 12CO J=1-0 indicates that there is a high-velocity molecular outflow near the IRAS19282+1814, which is blue mono-polar. Parameters of the outflow were calculated. The associated infrared source IRAS19282+1814 may be a massive young stellar object (YSO), which is embedded in the surrounding gas and dust according to the IRAS color indices. There is no other source nearby, so IRAS19282+1814 probably drives the outflow.

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