Characterization of the IRAS22129+7000 protostar and associated molecular outflow in B175 (=L1219)

Details Characterization of the IRAS22129+7000 protostar and associated molecular outflow in B175 (=L1219) Characterization of the IRAS22129+7000 protostar and associated molecular outflow in B175 (=L1219)

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sf2a.conf..233g&link_type=abstract

SF2A-2006: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: D. Barret, F. Casoli, G.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present a multi--wavelength study of the cold and deeply embedded IRAS22129+7000 source and associated bipolar outflow, first detected by Nikolic & Kun (2004), near the Ced201 reflection nebula. We have detected and resolved the source that drives the extended molecular outflow at high angular resolution using the IRAC camera and IRS spectrometer on board Spitzer, and mapped the 1.2 mm dust continuum emission with the MAMBO bolometer (at the IRAM--30m telescope). We have also mapped the outflow in the CO J=3-2 line with the Caltech Submillimeter Observatory (CSO) and targeted some specific positions in C18O, 13CO and HCO^+ (with the IRAM-30m), and in CO, DCO^+ and HCN (with the CSO).

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