Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-06-11
Astrophys.J. 593 (2003) L89-L92
Astronomy and Astrophysics
Astrophysics
7 pages including 1 figure. Submitted to ApJL. AAStex
Scientific paper
10.1086/378184
We present the result of astrometric observations of the radio pulsar PSR B0656+14, made using the Very Long Baseline Array. The parallax of the pulsar is pi = 3.47 +- 0.36 mas, yielding a distance of 288 +33 -27 pc. This independent distance estimate has been used to constrain existing models of thermal x-ray emission from the neutron star's photosphere. Simple blackbody fits to the x-ray data formally yield a neutron star radius R_inf ~ 7-8.5 km. With more realistic fits to a magnetized hydrogen atmosphere, any radius between ~13 and ~20 km is allowed.
Brisken Walter Frank
Golden Aaron
Goss William Miller
Thorsett Stephen. E.
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