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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3678

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DC Field	Value	Language
dc.contributor.author	Bhatt, H. C	-
dc.date.accessioned	2008-09-16T16:08:06Z	-
dc.date.available	2008-09-16T16:08:06Z	-
dc.date.issued	1990-06	-
dc.identifier.citation	Astronomy and Astrophysics , Vol. 232, No. 2, pp. 367 - 370	en
dc.identifier.issn	0004-6361	-
dc.identifier.uri	http://hdl.handle.net/2248/3678	-
dc.description.abstract	The 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.iso	en	en
dc.publisher	The European Southern Observatory	en
dc.relation.uri	http://ads.iucaa.ernet.in/abs/1990A%26A...232..367B	en
dc.subject	Molecular clouds	en
dc.subject	Pulsars	en
dc.subject	X ray stars	en
dc.subject	Binary stars	en
dc.subject	Infrared astronomy satellite	en
dc.subject	Stellar mass accretion	en
dc.subject	Stellar models	en
dc.subject	T tauri stars	en
dc.title	Is the X-ray pulsar H 0253 + 193 a neutron star spun down in a molecular cloud?	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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