Issue |
EAS Publications Series
Volume 52, 2011
Conditions and Impact of Star Formation
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Page(s) | 307 - 308 | |
DOI | https://doi.org/10.1051/eas/1152060 | |
Published online | 25 November 2011 |
M. Röllig, R. Simon, V. Ossenkopf and J. Stutzki (eds)
EAS Publications Series, 52 (2011) 307-308
Star Formation in the Orion A Molecular Cloud
1
e-mail: yoshito.shimajiri@nao.ac.jp
We present new, wide, and deep images in the AzTEC/ASTE 1.1 mm continuum and the 12 CO (J = 1–0) emission toward the northern part of the Orion-A GMC. We have found evidence for interactions between molecular clouds and the external forces that may trigger star formation. Two types of possible triggers were revealed: (1) Collisions of the diffuse gas on the cloud surface, particularly at the eastern side of the OMC-2/3 region, and (2) Irradiation of UV on the pre-existing filaments and dense molecular cloud cores. Our wide-field and high-sensitivity imaging has provided the first comprehensive view of the potential sites of triggered star formation in the Orion-A GMC.
© EAS, EDP Sciences 2011