Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822–371

Simple item page
dc.contributor.authorSomero, A
dc.contributor.authorHakala, P
dc.contributor.authorMuhli, P
dc.contributor.authorCharles, P
dc.contributor.authorVilhu, O
dc.date.accessioned2021-10-08T11:01:07Z
dc.date.available2021-10-08T11:01:07Z
dc.date.issued2012
dc.description.abstractContext. X1822–371 is the prototypical accretion disc corona X-ray source, a low-mass X-ray binary viewed at very high inclination, thereby allowing the disc structure and extended disc coronal regions to be visible. As the brightest (closest) such source, X1822–371 is ideal for studying the shape and edge structure of an accretion disc, and comparing with detailed models.
dc.identifier.apacitationSomero, A., Hakala, P., Muhli, P., Charles, P., & Vilhu, O. (2012). Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822–371. <i>Astronomy and Astrophysics</i>, 539(4), A111 - 177. http://hdl.handle.net/11427/35090en_ZA
dc.identifier.chicagocitationSomero, A, P Hakala, P Muhli, P Charles, and O Vilhu "Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822–371." <i>Astronomy and Astrophysics</i> 539, 4. (2012): A111 - 177. http://hdl.handle.net/11427/35090en_ZA
dc.identifier.citationSomero, A., Hakala, P., Muhli, P., Charles, P. & Vilhu, O. 2012. Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822–371. <i>Astronomy and Astrophysics.</i> 539(4):A111 - 177. http://hdl.handle.net/11427/35090en_ZA
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.ris TY - Journal Article AU - Somero, A AU - Hakala, P AU - Muhli, P AU - Charles, P AU - Vilhu, O AB - Context. X1822–371 is the prototypical accretion disc corona X-ray source, a low-mass X-ray binary viewed at very high inclination, thereby allowing the disc structure and extended disc coronal regions to be visible. As the brightest (closest) such source, X1822–371 is ideal for studying the shape and edge structure of an accretion disc, and comparing with detailed models. DA - 2012 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2012 SM - 0004-6361 SM - 1432-0746 T1 - Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822–371 TI - Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822–371 UR - http://hdl.handle.net/11427/35090 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/35090
dc.identifier.vancouvercitationSomero A, Hakala P, Muhli P, Charles P, Vilhu O. Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822–371. Astronomy and Astrophysics. 2012;539(4):A111 - 177. http://hdl.handle.net/11427/35090.en_ZA
dc.language.isoeng
dc.publisher.departmentDepartment of Astronomy
dc.publisher.facultyFaculty of Science
dc.sourceAstronomy and Astrophysics
dc.source.journalissue4
dc.source.journalvolume539
dc.source.paginationA111 - 177
dc.source.urihttps://dx.doi.org/10.1051/0004-6361/201118439
dc.subject.otherstars: individual:X1822–371
dc.subject.otheraccretion, accretion disks
dc.subject.otherX-rays: binaries
dc.subject.otheraccretion
dc.subject.otheraccretion disks
dc.titlePhase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822–371
dc.typeJournal Article
uct.type.publicationResearch
uct.type.resourceJournal Article
Files
Original bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
SomeroA_Phase_resolved_2012.pdf
Size:
516.18 KB
Format:
Adobe Portable Document Format
Description:
Download
Collections
Journal Articles