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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3925
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dc.contributor.authorBhatt, H. C-
dc.date.accessioned2008-10-15T10:21:44Z-
dc.date.available2008-10-15T10:21:44Z-
dc.date.issued1990-06-
dc.identifier.citationAstronomy and Astrophysics , Vol. 232, No. 2, pp. 367 - 370en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3925-
dc.description.abstractThe detection of 206s X-ray pulsations from H0253+193 indicates that the source is a compact object. It is argued here that object can not be a T Tauri star or Be/X –ray binary pulsar suggested that H 0253+193 is slowly rotating single neutron star now accreting interstellar matter after having been spun down by a propeller type mechanism during its passage through cloud.en
dc.language.isoenen
dc.publisherThe European Southern Observatoryen
dc.relation.urihttp://ads.iucaa.ernet.in/abs/1990A%26A...232..367Ben
dc.subjectMolecular cloudsen
dc.subjectPulsarsen
dc.subjectX ray starsen
dc.subjectBinary starsen
dc.subjectInfrared astronomy satelliteen
dc.subjectStellar mass accretionen
dc.subjectStellar modelsen
dc.subjectT tauri starsen
dc.titleIs the X-ray pulsar H 0253 + 193 a neutron star spun down in a molecular cloud?en
dc.typeArticleen
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