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An improved position for the X-ray source 3U0527-05

White, Glenn J. and Ricketts, Martin J. (1977). An improved position for the X-ray source 3U0527-05. Astrophysical Letters, 18(2) pp. 79–81.

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URL: http://adsabs.harvard.edu/abs/1977ApL....18...79W
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Abstract

An improved position is reported for the X-ray source 3U 0527-05. The two most likely optical counterparts are θ2 Orionis, a binary star system which contains a massive non luminous secondary, and the central regions of the Orion Nebula, M42. Upper limits to the X-ray emission from eight other binary systems which have a massive non luminous secondary component are given, based on analysis of data from the Ariel V X-ray satellite.

Item Type: Journal Article
Copyright Holders: 1977 Gordon and Breach Science Publishers Ltd., Taylor & Francis
ISSN: 0004-6388
Keywords: binary stars; nebulae; position errors; satellite observation; x-ray sources; light curve; protostars; spaceborne astronomy; x-ray astronomy; ariel satellites
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 33260
Depositing User: Glenn White
Date Deposited: 26 Mar 2012 09:15
Last Modified: 26 Mar 2012 09:49
URI: http://oro.open.ac.uk/id/eprint/33260
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