The large distance of GX5-1, suggested by the low-energy X-ray spectrum, restricts the number of possible optical candidates. A near infrared excess from the counterpart is expected.

Optical Candidates for the X-Ray Source GX 5-1 / Reina, C.; Tarenghi, M.. - In: ASTROPHYSICAL LETTERS. - ISSN 0004-6388. - 15:1(1973), pp. 7-8.

Optical Candidates for the X-Ray Source GX 5-1

Reina, C.;
1973

Abstract

The large distance of GX5-1, suggested by the low-energy X-ray spectrum, restricts the number of possible optical candidates. A near infrared excess from the counterpart is expected.
15
1
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http://adsabs.harvard.edu/full/1973ApL....15....7R
Reina, C.; Tarenghi, M.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/63295
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