OSSE observations of the Crab pulsar | Zendy

M. P. Ulmer | Zendy; S. Lomatch | Zendy; S. M. Matz | Zendy; D. A. Grabelsky | Zendy; W. R. Purcell | Zendy; J. E. Grove | Zendy; W. N. Johnson | Zendy; R. L. Kinzer | Zendy; J. D. Kurfess | Zendy; M. S. Strickman | Zendy; R. A. Cameron | Zendy; G. V. Jung | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

OSSE observations of the Crab pulsar

Author(s) -

M. P. Ulmer,

S. Lomatch,

S. M. Matz,

D. A. Grabelsky,

W. R. Purcell,

J. E. Grove,

W. N. Johnson,

R. L. Kinzer,

J. D. Kurfess,

M. S. Strickman,

R. A. Cameron,

G. V. Jung

Publication year - 1994

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/174564

Subject(s) - physics , pulsar , crab pulsar , astronomy , crab nebula , astrophysics

We present results of the Compton Gamma Ray Observatory OSSEobservations of the Crab pulsar, made during MJD 48373--48406 (27 April1991--30 May 1991) and MJD 48798--48804 (25 June 1992--1 July 1992). Pulsarlight curves and spectra over the 0.05 to 10 MeV range are presented. Thearrival time of the gamma-ray peak and the radio peak agree to within 30s,which is better than the 300s accuracy of the measurements. The overallpulse phase averaged spectrum in the 0.1--10 MeV range is well-fit ...

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research