COS-B identification of the new γ pulsar PSR 1055-52

Details COS-B identification of the new γ pulsar PSR 1055-52 COS-B identification of the new γ pulsar PSR 1055-52

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cha%26a..18..272s&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 18, Issue 3, p. 272-274.

Astronomy and Astrophysics

Astrophysics

Psr 1055, 52, Γ-Ray Pulsar, Timing Analysis

Scientific paper

Using COS-B data we analyzed the timing parameters of PSR 1055-52, the
newly discovered γ-ray pulsar by CGRO. We found a significant and
similar pulsed structure, thus confirming the CGRO discovery. A
comparison of this pulsar with 5 previously known ones is made.

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