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/2248/3925

Title:	Is the X-ray pulsar H 0253 + 193 a neutron star spun down in a molecular cloud?
Authors:	Bhatt, H. C
Keywords:	Molecular clouds Pulsars X ray stars Binary stars Infrared astronomy satellite Stellar mass accretion Stellar models T tauri stars
Issue Date:	Jun-1990
Publisher:	The European Southern Observatory
Citation:	Astronomy and Astrophysics , Vol. 232, No. 2, pp. 367 - 370
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.
URI:	http://hdl.handle.net/2248/3925
ISSN:	0004-6361
Appears in Collections:	IIAP Publications

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