Long-term orbital period variations for EU hydrae

Long-term period variations of an Algol-type eclipsing binary star, EU Hydrae, are presented based on an analysis of its O - C curve. As in the cases of other Algols studied in recent papers by one of the authors (S.-B. Qian), an alternate period change has discovered to superimpose on a secular per...

Full description

Saved in:
Bibliographic Details
Main Authors: Qian S.-B., Boonrucksar S.
Format: Article
Language:English
Published: 2014
Online Access:http://www.scopus.com/inward/record.url?eid=2-s2.0-30244467434&partnerID=40&md5=c31a187bb2c8192c853acb1624367985
http://cmuir.cmu.ac.th/handle/6653943832/6009
Tags: Add Tag
No Tags, Be the first to tag this record!
Institution: Chiang Mai University
Language: English
id th-cmuir.6653943832-6009
record_format dspace
spelling th-cmuir.6653943832-60092014-08-30T03:23:44Z Long-term orbital period variations for EU hydrae Qian S.-B. Boonrucksar S. Long-term period variations of an Algol-type eclipsing binary star, EU Hydrae, are presented based on an analysis of its O - C curve. As in the cases of other Algols studied in recent papers by one of the authors (S.-B. Qian), an alternate period change has discovered to superimpose on a secular period decrease (dP/dt = -4.8 × 10-8 dyr-1). By assuming that the alternate variation is cyclic, a period of 26.5 yr and an amplitude of 0.0104 d were determined. A long-term period decrease combined with a semi-detached configuration may indicate that EU Hya is undergoing a secular angular momentum loss. Three possible mechanisms are proposed to explain the alternate period change. 2014-08-30T03:23:44Z 2014-08-30T03:23:44Z 2003 Article 00046264 http://www.scopus.com/inward/record.url?eid=2-s2.0-30244467434&partnerID=40&md5=c31a187bb2c8192c853acb1624367985 http://cmuir.cmu.ac.th/handle/6653943832/6009 English
institution Chiang Mai University
building Chiang Mai University Library
country Thailand
collection CMU Intellectual Repository
language English
description Long-term period variations of an Algol-type eclipsing binary star, EU Hydrae, are presented based on an analysis of its O - C curve. As in the cases of other Algols studied in recent papers by one of the authors (S.-B. Qian), an alternate period change has discovered to superimpose on a secular period decrease (dP/dt = -4.8 × 10-8 dyr-1). By assuming that the alternate variation is cyclic, a period of 26.5 yr and an amplitude of 0.0104 d were determined. A long-term period decrease combined with a semi-detached configuration may indicate that EU Hya is undergoing a secular angular momentum loss. Three possible mechanisms are proposed to explain the alternate period change.
format Article
author Qian S.-B.
Boonrucksar S.
spellingShingle Qian S.-B.
Boonrucksar S.
Long-term orbital period variations for EU hydrae
author_facet Qian S.-B.
Boonrucksar S.
author_sort Qian S.-B.
title Long-term orbital period variations for EU hydrae
title_short Long-term orbital period variations for EU hydrae
title_full Long-term orbital period variations for EU hydrae
title_fullStr Long-term orbital period variations for EU hydrae
title_full_unstemmed Long-term orbital period variations for EU hydrae
title_sort long-term orbital period variations for eu hydrae
publishDate 2014
url http://www.scopus.com/inward/record.url?eid=2-s2.0-30244467434&partnerID=40&md5=c31a187bb2c8192c853acb1624367985
http://cmuir.cmu.ac.th/handle/6653943832/6009
_version_ 1681420533162311680