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Search for continuous X-ray emission from NP 0532A search for continuous X-ray emission from the pulsar NP 0532 has been performed using lunar occultations and high temporal resolution. No increase in the nonpulsed phase of the flux from the Crab Nebula was observed when NP 0532 was exposed. The result is used to establish an upper limit of 4.7 million K (99% confidence) on the surface temperature of the neutron star.
Document ID
19760033069
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/181985
Authors
Wolff, R. S. (Columbia Univ. New York, NY, United States)
Kestenbaum, H. L. (Columbia Univ. New York, NY, United States)
Ku, W. (Columbia Univ. New York, NY, United States)
Novick, R. (Columbia University New York, N.Y., United States)
Date Acquired
August 8, 2013
Publication Date
December 1, 1975
Publication Information
Publication: Astrophysical Journal
Volume: 202
Subject Category
Astrophysics
Accession Number
76A16035
Funding Number(s)
CONTRACT_GRANT: NSF MPS-74-05924A01
CONTRACT_GRANT: NGR-33-008-102
Distribution Limits
Public
Copyright
Other

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