Two micron spectroscopy of infrared sources in NGC 2071

Details Two micron spectroscopy of infrared sources in NGC 2071 Two micron spectroscopy of infrared sources in NGC 2071

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...377..246w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 377, Aug. 10, 1991, p. 246-249.

Astronomy and Astrophysics

Astronomy

27

H Ii Regions, Infrared Sources (Astronomy), Infrared Spectra, Reflection Nebulae, Star Formation, Carbon Monoxide, Emission Spectra, Line Spectra

Scientific paper

2.10-2.35 micron spectra of seven compact infrared sources in the central region of the bipolar outflow NGC 2071 are presented. Line emission from CO at the wavelengths of the 2-0, 3-1, and 4-2 band heads has been detected in IRS 1 and IRS 7. In addition, Br-gamma line emission is present in IRS 1. It is suggested that the NGC 2071 bipolar outflow is a composite of two or more outflows.

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