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Understanding the LMXB X2127+119 in M 15. II. The UV data

dc.contributor.authorIoannou, Z
dc.contributor.authorvan Zyl, L
dc.contributor.authorNaylor, T
dc.contributor.authorCharles, PA
dc.contributor.authorMargon, B
dc.contributor.authorKoch-Miramond, L
dc.contributor.authorIlovaisky, S
dc.date.accessioned2018-02-13T14:45:43Z
dc.date.issued2003-02-01
dc.description.sponsorshipLvZ acknowledges the support of scholarships from the Vatican Observatory, the National Research Foundation (South Africa), the University of Cape Town, and the Overseas Research Studentship scheme (UK). TN was in receipt of a PPARC advanced fellowship when the majority of this work was carried out.en_GB
dc.identifier.citationVol. 399 (1), pp. 211 - 218en_GB
dc.identifier.doi10.1051/0004-6361:20021578
dc.identifier.urihttp://hdl.handle.net/10871/31452
dc.language.isoenen_GB
dc.publisherEDP Sciences for European Southern Observatory (ESO)en_GB
dc.rights© ESO 2003en_GB
dc.subjectaccretionen_GB
dc.subjectaccretion discsen_GB
dc.subjectstars: individual: X2127+119en_GB
dc.subjectstars: coronaeen_GB
dc.subjectAC211en_GB
dc.subjectultraviolet: starsen_GB
dc.subjectstars: binaries: eclipsingen_GB
dc.titleUnderstanding the LMXB X2127+119 in M 15. II. The UV dataen_GB
dc.typeArticleen_GB
dc.date.available2018-02-13T14:45:43Z
dc.descriptionThis is the author accepted manuscript. The final version is available from EDP Sciences via the DOI in this recorden_GB
dc.identifier.journalAstronomy and Astrophysicsen_GB


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