NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login

Due to the lapse in federal government funding, NASA is not updating this website. We sincerely regret this inconvenience.

Back to Results
The 4U 0115+63: Another energetic gamma ray binary pulsarFollowing the discovery of Her X-1 as a source of pulsed 1000 Gev X-rays, a search for emission from an X-ray binary containing a pulsar with similar values of period, period derivative and luminosity was successful. The sporadic X-ray binary 4U 0115-63 has been observed, with probability 2.5 x 10 to the minus 6 power ergs/s to emit 1000 GeV gamma-rays with a time averaged energy flux of 6 to 10 to the 35th power.
Document ID
19850025660
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Chadwick, P. M. (Durham Univ.)
Dipper, N. A. (Durham Univ.)
Dowthwaite, J. C. (Durham Univ.)
Kirkman, I. W. (Durham Univ.)
Mccomb, T. J. L. (Durham Univ.)
Orford, K. J. (Durham Univ.)
Turver, K. E. (Durham Univ.)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 1
Subject Category
Space Radiation
Report/Patent Number
OG-2.6-11
Report Number: OG-2.6-11
Accession Number
85N33973
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Related Records

IDRelationTitle19850025589Collected WorksNinteenth International Cosmic Ray Conference. OG Sessions, Volume 119850025589Collected WorksNinteenth International Cosmic Ray Conference. OG Sessions, Volume 1
No Preview Available