NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
New infrared-CO source in M8A far-infrared map of the M8 region at 69 microns with a 1-arcmin resolution shows an unresolved source 19 arcmin east of the main component. This source is a strong near-infrared emitter, with K = 4.8 and K - L = 2.6 mag. An intense peak in (C-12)O emission (brightness temperature about 36 K) coincides with the new infrared source. Comparison of millimeter-wave and infrared observations suggest that this source is an extremely young compact H II region. Evidence for a depletion of dust opacity inside the H II region is also found.
Document ID
19770047985
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Wright, E. L.
(Arizona Univ. Tucson, AZ, United States)
Lada, C. J.
(Arizona Univ. Tucson, AZ, United States)
Fazio, G. G.
(Harvard College Observatory and Smithsonian Astrophysical Observatory Cambridge, Mass., United States)
Low, F. J.
(Arizona, University Tucson, Ariz., United States)
Kleinmann, D. E.
(Arizona Univ. Tucson, AZ, United States)
Date Acquired
August 8, 2013
Publication Date
February 1, 1977
Publication Information
Publication: Astronomical Journal
Volume: 82
Subject Category
Astrophysics
Accession Number
77A30837
Funding Number(s)
CONTRACT_GRANT: NGR-22-007-270
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available