High-velocity HCO(+) emission from L1551 IRS 5 - Evidence for wind-cloud interactions

Details High-velocity HCO(+) emission from L1551 IRS 5 - Evidence for wind-cloud interactions High-velocity HCO(+) emission from L1551 IRS 5 - Evidence for wind-cloud interactions

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...397l.111r&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 397, no. 2, p. L111-L114.

Astronomy and Astrophysics

Astronomy

17

Clumps, Formyl Ions, Interstellar Matter, Plasma Jets, Star Formation, Stellar Envelopes, Abundance, Brightness Temperature, Infrared Sources (Astronomy), Morphology

Scientific paper

Interferometric HCO(+) observations of the region surrounding IRS 5 were made to search for high-velocity gas and for stationary gas associated with the L1551 optical jet. The discovery of -50 km/s gas from IRS 5 is reported along with stationary clumps of material surrounding the L1551 optical jet. The clumps may be the material against which the wind from IRS 5 is being shocked, producing the optical jet. The clumps are probably part of a larger structure, possibly the walls of a cavity swept out by the wind from IRS 5.

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