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

We made mapping observation in the 12CO J=1-0 line which revealed the existence of a blue-shifted monopolar high-velocity molecular outflow near IRAS19292+1814. The parameters of this outflow are calculated. As indicated by the IRAS color indices, the associated infrared source IRAS19292+1814 may be...

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Published inChinese astronomy and astrophysics Vol. 27; no. 1; pp. 73 - 78
Main Authors Sun, Ke-feng, Wu, Yue-fang
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.01.2003
Subjects
formation
infrared
ISM
jets
outflows
stars
ISM
infrared
outflows
stars
jets
formation
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Abstract We made mapping observation in the 12CO J=1-0 line which revealed the existence of a blue-shifted monopolar high-velocity molecular outflow near IRAS19292+1814. The parameters of this outflow are calculated. As indicated by the IRAS color indices, the associated infrared source IRAS19292+1814 may be a massive young stellar object (YSO) deeply embedded in the surrounding gas and dust. There is no other source nearby, so IRAS19292+1814 probably is the driving source of the outflow.
AbstractList We made mapping observation in the 12CO J=1-0 line which revealed the existence of a blue-shifted monopolar high-velocity molecular outflow near IRAS19292+1814. The parameters of this outflow are calculated. As indicated by the IRAS color indices, the associated infrared source IRAS19292+1814 may be a massive young stellar object (YSO) deeply embedded in the surrounding gas and dust. There is no other source nearby, so IRAS19292+1814 probably is the driving source of the outflow.
We made mapping observation in the 12CO J=1-0 line which revealed the existence of a blue-shifted monopolar high-velocity molecular outflow near IRAS19292+1814. The parameters of this outflow are calculated. As indicated by the IRAS color indices, the associated infrared source IRAS19292+1814 may be a massive young stellar object (YSO) deeply embedded in the surrounding gas and dust. There is no other source nearby, so IRAS19292+1814 probably is the driving source of the outflow.
Author Sun Ke-feng
Wu Yue-fang
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Cites_doi 10.1086/160723
10.1086/168261
10.1086/181613
10.1086/167390
10.1146/annurev.aa.23.090185.001411
10.1086/162635
10.1086/178057
10.1051/0004-6361:20011498
10.1086/191522
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Snippet We made mapping observation in the 12CO J=1-0 line which revealed the existence of a blue-shifted monopolar high-velocity molecular outflow near...
We made mapping observation in the 12CO J=1-0 line which revealed the existence of a blue-shifted monopolar high-velocity molecular outflow near...
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SubjectTerms formation
infrared
ISM
jets
outflows
stars
Title A new high-velocity molecular outflow of IRAS 19282+1814
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