Is the X-ray pulsar H 0253 + 193 a neutron star spun down in a molecular cloud?

Details Is the X-ray pulsar H 0253 + 193 a neutron star spun down in a molecular cloud? Is the X-ray pulsar H 0253 + 193 a neutron star spun down in a molecular cloud?

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...232..367b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 232, no. 2, June 1990, p. 367-370.

Astronomy and Astrophysics

Astronomy

8

Molecular Clouds, Pulsars, X Ray Stars, Binary Stars, Infrared Astronomy Satellite, Stellar Mass Accretion, Stellar Models, T Tauri Stars, X-Ray Pulsars, Propeller Spin Down, Interstellar Medium: Clouds, Accretion

Scientific paper

The detection of 206s X-ray pulsations from H 0253 + 193 indicates that the source is a compact object. It is argued here that the object can not be a T Tauri star or a Be/X-ray binary pulsar embedded in the molecular cloud L 1457. It is suggested that H 0253+193 is a slowly rotating single neutron star now accreting interstellar matter after having been spun down by a propeller type mechanism during its passage through the cloud.

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