Spectroscopic Study of the Early-Type Binary HX Vel A
| dc.authorid | Soydugan, Faruk / 0000-0002-5141-7645 | |
| dc.authorid | Özkardeş, Burcu / 0000-0002-6764-9299 | |
| dc.authorid | Sürgit, Derya / 0000-0002-0303-3516 | |
| dc.authorid | Erdem, Ahmet / 0000-0001-5289-8850 | |
| dc.authorid | Soydugan, Faruk / 0000-0002-5141-7645 | |
| dc.authorid | Demircan, Osman / 0000-0002-2365-642X | |
| dc.contributor.author | Özkardeş, Burcu | |
| dc.contributor.author | Sürgit, Derya | |
| dc.contributor.author | Erdem, Ahmet | |
| dc.contributor.author | Budding, Edwin | |
| dc.contributor.author | Soydugan, Faruk | |
| dc.contributor.author | Demircan, Osman | |
| dc.date.accessioned | 2025-01-27T21:06:04Z | |
| dc.date.available | 2025-01-27T21:06:04Z | |
| dc.date.issued | 2012 | |
| dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
| dc.description | 282nd Symposium of the International-Astronomical-Union -- JUL 18-22, 2011 -- Tatranska Lomnica, SLOVAKIA | |
| dc.description.abstract | This paper presents high resolution spectroscopy of the HX Vel (IDS 08390-4744 AB) multiple system. New spectroscopic observations of the system were made at Mt. John University Observatory in 2007 and 2008. Radial velocities of both components of HX Vel A were measured using gaussian fitting. The spectroscopic mass ratio of the close binary was determined as 0.599 +/- 0.052, according to a Keplerian orbital solution. The resulting orbital elements are a(1)sini=0.0098 +/- 0.0003 AU, a(2)sini=0.0164 +/- 0.0003 AU, M(1)sin(3)i=1.19 +/- 0.07 M-circle dot and M(2)sin(3)i=0.71 +/- 0.04 M-circle dot. | |
| dc.description.sponsorship | Int Astronom Union,Slovak Acad Sci, Astronom Inst,SUH Slovak Central Observ,TESCO Poprad,Sintra Poprad,Papyrus Poprad,Town Vysoke Tatry,Town Poprad,High Tatras Tourism Assoc,Nord Svit,Buntavar Svit | |
| dc.identifier.doi | 10.1017/S1743921311026925 | |
| dc.identifier.endpage | + | |
| dc.identifier.isbn | 978-1-107-01982-9 | |
| dc.identifier.issn | 1743-9213 | |
| dc.identifier.issn | 1743-9221 | |
| dc.identifier.issue | 282 | |
| dc.identifier.scopus | 2-s2.0-84887397083 | |
| dc.identifier.scopusquality | Q4 | |
| dc.identifier.startpage | 67 | |
| dc.identifier.uri | https://doi.org/10.1017/S1743921311026925 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.12428/27890 | |
| dc.identifier.wos | WOS:000309244400016 | |
| dc.identifier.wosquality | N/A | |
| dc.indekslendigikaynak | Web of Science | |
| dc.indekslendigikaynak | Scopus | |
| dc.language.iso | en | |
| dc.publisher | Cambridge Univ Press | |
| dc.relation.ispartof | From Interacting Binaries To Exoplanets: Essential Modeling Tools | |
| dc.relation.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | |
| dc.rights | info:eu-repo/semantics/closedAccess | |
| dc.snmz | KA_WoS_20250125 | |
| dc.subject | methods: data analysis | |
| dc.subject | techniques: spectroscopic | |
| dc.subject | stars: early-type | |
| dc.subject | (stars:) binaries (including multiple): close | |
| dc.subject | stars: individual (HX Vel A) | |
| dc.title | Spectroscopic Study of the Early-Type Binary HX Vel A | |
| dc.type | Conference Object |
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