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Protostellar Candidates in W75N

Published online by Cambridge University Press:  04 August 2017

C. M. Mountain ,
I. Gatley ,
T. W. Hartquist ,
S. K. Leggett  and
M. J. Selby
C. M. Mountain
Affiliation:
UKIRT, 900 Leilani St., Hilo, HI 96720, USA
I. Gatley
Affiliation:
UKIRT, 900 Leilani St., Hilo, HI 96720, USA
T. W. Hartquist
Affiliation:
UKIRT, 900 Leilani St., Hilo, HI 96720, USA
S. K. Leggett
Affiliation:
UKIRT, 900 Leilani St., Hilo, HI 96720, USA
M. J. Selby
Affiliation:
UKIRT, 900 Leilani St., Hilo, HI 96720, USA

Extract

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W75N is a highly obscured region containing far-infrared sources, masers and molecular clouds. New results are presented showing highly reddened point sources near the maser source W75N(OH). One of these sources appears to be illuminating a newly discovered reflection nebula exhibiting large scale fluorescent molecular hydrogen.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 187
Copyright
Copyright © Reidel 1987