Long-term evolution of the neutron-star spin period of SXP 1062

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dc.contributor.authorSturm, R
dc.contributor.authorHaberl, F
dc.contributor.authorOskinova, L M
dc.contributor.authorSchurch, M P E
dc.contributor.authorHénault-Brunet, V
dc.contributor.authorGallagher, J S
dc.contributor.authorUdalski, A
dc.date.accessioned2021-10-08T11:01:09Z
dc.date.available2021-10-08T11:01:09Z
dc.date.issued2013
dc.description.abstractContext. The Be/X-ray binary SXP 1062 is of especial interest owing to the large spin period of the neutron star, its large spin-down rate, and the association with a supernova remnant constraining its age. This makes the source an important probe for accretion physics.
dc.identifier.apacitationSturm, R., Haberl, F., Oskinova, L. M., Schurch, M. P. E., Hénault-Brunet, V., Gallagher, J. S., & Udalski, A. (2013). Long-term evolution of the neutron-star spin period of SXP 1062. <i>Astronomy and Astrophysics</i>, 556(4), A139 - 177. http://hdl.handle.net/11427/35098en_ZA
dc.identifier.chicagocitationSturm, R, F Haberl, L M Oskinova, M P E Schurch, V Hénault-Brunet, J S Gallagher, and A Udalski "Long-term evolution of the neutron-star spin period of SXP 1062." <i>Astronomy and Astrophysics</i> 556, 4. (2013): A139 - 177. http://hdl.handle.net/11427/35098en_ZA
dc.identifier.citationSturm, R., Haberl, F., Oskinova, L.M., Schurch, M.P.E., Hénault-Brunet, V., Gallagher, J.S. & Udalski, A. 2013. Long-term evolution of the neutron-star spin period of SXP 1062. <i>Astronomy and Astrophysics.</i> 556(4):A139 - 177. http://hdl.handle.net/11427/35098en_ZA
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.ris TY - Journal Article AU - Sturm, R AU - Haberl, F AU - Oskinova, L M AU - Schurch, M P E AU - Hénault-Brunet, V AU - Gallagher, J S AU - Udalski, A AB - Context. The Be/X-ray binary SXP 1062 is of especial interest owing to the large spin period of the neutron star, its large spin-down rate, and the association with a supernova remnant constraining its age. This makes the source an important probe for accretion physics. DA - 2013 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2013 SM - 0004-6361 SM - 1432-0746 T1 - Long-term evolution of the neutron-star spin period of SXP 1062 TI - Long-term evolution of the neutron-star spin period of SXP 1062 UR - http://hdl.handle.net/11427/35098 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/35098
dc.identifier.vancouvercitationSturm R, Haberl F, Oskinova LM, Schurch MPE, Hénault-Brunet V, Gallagher JS, et al. Long-term evolution of the neutron-star spin period of SXP 1062. Astronomy and Astrophysics. 2013;556(4):A139 - 177. http://hdl.handle.net/11427/35098.en_ZA
dc.language.isoeng
dc.publisher.departmentDepartment of Astronomy
dc.publisher.facultyFaculty of Science
dc.sourceAstronomy and Astrophysics
dc.source.journalissue4
dc.source.journalvolume556
dc.source.paginationA139 - 177
dc.source.urihttps://dx.doi.org/10.1051/0004-6361/201321755
dc.subject.otherpulsars: individual: SXP1062
dc.subject.othergalaxies: individual: Small Magellanic Cloud
dc.subject.otherstars: emission-line, Be
dc.subject.otherstars: neutron
dc.subject.otherX-rays: binaries
dc.subject.otherstars: emission-line
dc.subject.otherBe
dc.titleLong-term evolution of the neutron-star spin period of SXP 1062
dc.typeJournal Article
uct.type.publicationResearch
uct.type.resourceJournal Article
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