Interaction between the outflow and the core in IRAM 04191+1522

Details Interaction between the outflow and the core in IRAM 04191+1522 Interaction between the outflow and the core in IRAM 04191+1522

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..421t&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 8, p. 421 - 427 (2003)

Astronomy and Astrophysics

Astronomy

Protostars, Outflows, Molecular Clouds

Scientific paper

We have carried out mapping observations of the molecular cloud core associated with the young protostar, IRAM 04191+1522, in the CH3OH line. We have discovered interaction regions between the core and the outflow from the protostar. The interaction regions in IRAM 04191+1522 are not shocked regions as found in the previous studies of interaction between cores and outflows, but "quiescent" interaction regions. Our observational studies have revealed that interaction between cores and outflows takes place at the very early stage of protostellar formation, and that such interaction could greatly affect the final stellar mass of the protostar.

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