NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login

Press Enter or click the Search button to begin your search.

Back to Results
Strong source VLBI observations at 22 GHzTwenty-six strong high-frequency radio sources have been observed at 22.3 GHz on interferometer baselines of approximately 500 million wavelengths. Twenty-five were detected, and 14 have mean visibilities over 50 percent. The strongest sources as a group are more heavily resolved than the weaker sources.
Document ID
19860026126
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/163464
Authors
Lawrence, C. R. (California Inst. of Tech. Pasadena, CA, United States)
Readhead, A. C. S. (California Institute of Technology Pasadena, United States)
Linfield, R. P. (California Inst. of Tech. Pasadena, CA, United States)
Payne, D. G. (California Inst. of Tech. Pasadena, CA, United States)
Preston, R. A. (California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 12, 2013
Publication Date
September 15, 1985
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 296
ISSN: 0004-637X
Subject Category
Astronomy
Report/Patent Number
ISSN: 0004-637X
Accession Number
86A10864
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.

Related Records

There are no records associated with this record.
No Preview Available