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Two micron spectroscopy of infrared sources in NGC 2071

Journal Article · · Astrophysical Journal; (United States)
DOI:https://doi.org/10.1086/170352· OSTI ID:5223966
; ;  [1]
  1. Joint Astronomy Centre, Hilo, HI (United States) Lancashire Polytechnic, Preston (England)
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. 16 refs.
OSTI ID:
5223966
Journal Information:
Astrophysical Journal; (United States), Journal Name: Astrophysical Journal; (United States) Vol. 377; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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