First Spectroscopic Solutions of Two Southern Eclipsing Binaries: HO Tel and QY Tel

Basit Öğe Kaydı
dc.contributor.authorSurgit, D.
dc.contributor.authorErdem, A.
dc.contributor.authorEngelbrecht, C. A.
dc.contributor.authorvan Heerden, P.
dc.contributor.authorManick, R.
dc.date.accessioned2025-01-27T21:07:29Z
dc.date.available2025-01-27T21:07:29Z
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 preliminary results from the analysis of spectroscopic observations of two southern eclipsing binary stars, HO Tel and QY Tel. The grating spectra of these two systems were obtained at the Sutherland Station of the South African Astronomical Observatory in 2013. Radial velocities of the components were determined by the Fourier disentangling technique. Keplerian radial velocity models of HO Tel and QY Tel give their mass ratio as 0.921 +/- 0.005 and 1.089 +/- 0.007, respectively.
dc.description.sponsorshipSci Org Comm
dc.identifier.endpage259
dc.identifier.isbn978-1-58381-877-0
dc.identifier.isbn978-1-58381-876-3
dc.identifier.startpage258
dc.identifier.urihttps://hdl.handle.net/20.500.12428/28071
dc.identifier.volume496
dc.identifier.wosWOS:000369467900050
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.titleFirst Spectroscopic Solutions of Two Southern Eclipsing Binaries: HO Tel and QY Tel
dc.typeConference Object

Dosyalar

Koleksiyon

WoS İndeksli Yayınlar Koleksiyonu