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Infrared CO Emission from WL 16

Published online by Cambridge University Press:  04 August 2017

Rodger I. Thompson
Rodger I. Thompson*
Affiliation:
Steward Observatory, University of Arizona, Tucson, AZ 85721, USA

Extract

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The Rho Ophiuchi source WL 16 is the second Young Stellar Object (YSO) found to have infrared CO emission bands. IRAS observations show that WL 16 is far less luminous (∼ 14 L⊙) than the first source of infrared CO emission, BN (> 5000 L⊙). Also in contrast to BN, the CO emission from WL 16 represents a significant fraction of the total luminosity. The 2.3 μm first overtone CO emission bands were observed with the Steward Observatory Fourier Transform Spectrometer at the 2.3 m telescope.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 74 - 75
Copyright
Copyright © Reidel 1987