New Spectroscopic Solution of the Eclipsing Binary HX Vel A

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dc.contributor.authorSurgit, Derya
dc.contributor.authorErdem, Ahmet
dc.contributor.authorOzkardes, Burcu
dc.contributor.authorButland, Roger
dc.contributor.authorBudding, Edwin
dc.date.accessioned2025-01-27T21:00:01Z
dc.date.available2025-01-27T21:00:01Z
dc.date.issued2015
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionConference on Living Together: Planets, Host Stars and Binaries -- SEP 08-12, 2014 -- Litomysl, CZECH REPUBLIC
dc.description.abstractWe present a preliminary analysis of new spectroscopic observations of the southern binary HX Vel A. High-resolution spectroscopic observations were made at the Mt. John University Observatory in 2014. Radial velocities for HX Vel A were determined from the Gaussian profile-fitting method. The Keplerian radial velocity model gives the close binary mass ratio as 0.57 +/- 0.06. The resulting orbital elements are ai sin i = 0.0086 +/- 0.0003 au, a(2) sin i = 0.0151 +/- 0.0003 au, M-1 sin(3) i = 0.887 +/- 0.046 M-circle dot, and M-2 sin(3) i = 0.504 +/- 0.032 M-circle dot.
dc.description.sponsorshipSci Org Comm
dc.identifier.endpage261
dc.identifier.isbn978-1-58381-877-0
dc.identifier.isbn978-1-58381-876-3
dc.identifier.startpage260
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26912
dc.identifier.volume496
dc.identifier.wosWOS:000369467900051
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherAstronomical Soc Pacific
dc.relation.ispartofLiving Together: Planets, Host Stars, and Binaries
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectStars
dc.titleNew Spectroscopic Solution of the Eclipsing Binary HX Vel A
dc.typeConference Object

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