Soft X-ray observations of the radio pulsar PSR 1055-52

Details Soft X-ray observations of the radio pulsar PSR 1055-52 Soft X-ray observations of the radio pulsar PSR 1055-52

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...182...71b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 182, no. 1, Aug. 1987, p. 71-74. DFG-supported research.

Astronomy and Astrophysics

Astrophysics

37

Neutron Stars, Pulsars, Radio Stars, X Ray Sources, Cooling, Exosat Satellite, Stellar Spectra, Stellar Temperature, Thermal Emission

Scientific paper

The radio pulsar PSR 1055-52 was observed with the EXOSAT X-ray
satellite for a total of 105 s. The data can be fitted best
with blackbody spectra having temperatures of 5×105
≤ T ≤ 8×105K. The obtained temperatures are
consistent with recent models for the initial cooling of neutron stars.

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