NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
On the relationship between the infrared source CRL 2591 /UOA-27/ and its radio and H2O counterpartsRecent radio, infrared, and H2O maser observations show that there is a 7-arcsec angular separation between the protostarlike infrared source CRL 2591 and the compact H II region which has until now been identified with it, while the H2O maser coincides with the infrared source. This result, together with an extension of photometric measurements to 20 microns and a much improved upper limit to its angular size, reinforces the apparent similarity of CRL 2591 to the BN object in Orion and to W3/IRS 5.
Document ID
19770038230
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Wynn-Williams, C. G.
(California Inst. of Tech. Pasadena, CA, United States)
Forster, J. R.
(California Inst. of Tech. Pasadena, CA, United States)
Welch, W. J.
(California Inst. of Tech. Pasadena, CA, United States)
Wright, M. C. H.
(California, University Berkeley, Calif., United States)
Matthews, K.
(California Institute of Technology Pasadena, Calif., United States)
Becklin, E. E.
(California Inst. of Tech. Pasadena, CA, United States)
Neugebauer, G.
(California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 9, 2013
Publication Date
January 15, 1977
Publication Information
Publication: Astrophysical Journal
Volume: 211
Subject Category
Astronomy
Accession Number
77A21082
Funding Number(s)
CONTRACT_GRANT: NSF AST-76-22480
CONTRACT_GRANT: NSF MPS-74-18555-A01
CONTRACT_GRANT: NGL-05-002-207
Distribution Limits
Public
Copyright
Other

Available Downloads

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