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Submillimeter-wave observations of outflow and envelope around the low mass protostar IRAS 13036-7644

  • Kazuhisa Kamegai (a1), Masaaki Hiramatsu (a2), Takahiro Hayakawa (a3), Ken'ichi Tatematsu (a3), Tetsuo Hasegawa (a3), Toshikazu Onishi (a4) and Akira Mizuno (a5)...

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The interaction between molecular outflow from a protostar and ambient molecular cloud would play an important role in dissipating circumstellar envelope, changing chemical composition, and triggering next generation star formation. In order to investigate the interaction in submillimeter wavelength, we have made line observations toward the low mass protostar IRAS 13036-7644 (Class 0/I) in the Cha II dark cloud. Although millimeter observations found CO outflow and evidence of mass infall toward the protostar (e.g. Lehtinen 1997), no submillimeter observation has been reported so far.

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Lehtinen, K. 1997, A&A 317, L5
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Submillimeter-wave observations of outflow and envelope around the low mass protostar IRAS 13036-7644

  • Kazuhisa Kamegai (a1), Masaaki Hiramatsu (a2), Takahiro Hayakawa (a3), Ken'ichi Tatematsu (a3), Tetsuo Hasegawa (a3), Toshikazu Onishi (a4) and Akira Mizuno (a5)...

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