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Reanalysis of the orbital period variations of two DLMR overcontact binaries:FG Hya and GR Vir
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  • 英文篇名:Reanalysis of the orbital period variations of two DLMR overcontact binaries:FG Hya and GR Vir
  • 作者:Xu-Dong ; Zhang ; Yun-Xia ; Yu ; Fu-Yuan ; Xiang ; Ke ; Hu
  • 英文作者:Xu-Dong Zhang;Yun-Xia Yu;Fu-Yuan Xiang;Ke Hu;Department of Physics,Xiangtan University;
  • 英文关键词:binaries:close;;binaries:eclipsing;;stars:individual(FG Hya,GR Vir)
  • 中文刊名:TTWL
  • 英文刊名:天文和天体物理学研究(英文版)
  • 机构:Department of Physics,Xiangtan University;
  • 出版日期:2017-12-15
  • 出版单位:Research in Astronomy and Astrophysics
  • 年:2017
  • 期:v.17
  • 基金:supported by the National Natural Science Foundation of China (Grant No.11703020);; Joint Research Funds in Astronomy (U1531108,U1731106 and U1731110) under cooperative agreement between the National Natural Science Foundation of China and Chinese Academy of Sciences
  • 语种:英文;
  • 页:TTWL201712010
  • 页数:6
  • CN:12
  • ISSN:11-5721/P
  • 分类号:97-102
摘要
We investigate orbital period changes of two deep, low mass ratio(DLMR) overcontact W UMa-type binaries, FG Hya and GR Vir. It is found that the orbital period of FG Hya shows a cyclic change with a period of P_(mod)= 54.44 yr. The cyclic oscillation may be due to a third body in an eccentric orbit, while the orbital period of GR Vir shows a periodic variation with a period of P_(mod)= 28.56 yr and an amplitude of A = 0.0352 d. The periodic variation of GR Vir can be interpreted as a result of either the light-time effect of an unseen third body or the magnetic activity cycle.
        We investigate orbital period changes of two deep, low mass ratio(DLMR) overcontact W UMa-type binaries, FG Hya and GR Vir. It is found that the orbital period of FG Hya shows a cyclic change with a period of P_(mod)= 54.44 yr. The cyclic oscillation may be due to a third body in an eccentric orbit, while the orbital period of GR Vir shows a periodic variation with a period of P_(mod)= 28.56 yr and an amplitude of A = 0.0352 d. The periodic variation of GR Vir can be interpreted as a result of either the light-time effect of an unseen third body or the magnetic activity cycle.
引文
Agerer,F.,&Hubscher,J.1996,Information Bulletin on Variable Stars,4383
    Applegate,J.H.1992,Ap J,385,621
    Binnendijk,L.1963,AJ,68,30
    Cereda,L.,Misto,A.,Poretti,E.,&Niarchos,P.G.1988,A&AS,76,255
    Halbedel,E.M.1988,Information Bulletin on Variable Stars,3132
    Harris,A.W.1979,Information Bulletin on Variable Stars,1691
    Hoffmeister,C.1934,Astronomische Nachrichten,253,195
    Hubscher,J.,Lehmann,P.B.,&Walter,F.2012,Information Bulletin on Variable Stars,6010
    Kreiner,J.M.2004,Acta Astronomica,54,207
    Lafta,S.J.,&Grainger,J.F.1986,Ap&SS,127,153
    Lanza,A.F.,Rodono,M.,&Rosner,R.1998,MNRAS,296,893
    Lu,W.,&Rucinski,S.M.1999,AJ,118,515
    Mahdy,H.A.,Hamdy,M.A.,&Soliman,M.A.1985,Information Bulletin on Variable Stars,2811
    Ogloza,W.,Niewiadomski,W.,Barnacka,A.,et al.2008,Information Bulletin on Variable Stars,5843
    Qian,S.,Liu,Q.,&Yang,Y.1999,A&A,341,799
    Qian,S.-B.,&Yang,Y.-G.2004,AJ,128,2430
    Qian,S.-B.,He,J.,Xiang,F.,Ding,X.,&Boonrucksar,S.2005,AJ,129,1686
    Qian,S.,&Yang,Y.2005,MNRAS,356,765
    Rucinski,S.M.,&Lu,W.1999,AJ,118,2451
    Samolyk,G.2012,Journal of the American Association of Variable Star Observers(JAAVSO),40,975
    Smith,H.J.1955,AJ,60,179
    Smith,H.J.1963,AJ,68,39
    Strohmeier,W.,Knigge,R.,&Ott,H.1965,Information Bulletin on Variable Stars,115
    Tsesevich,V.P.1949,Peremennye Zvezdy 7,8
    Vinko,J.1989,Diploma-Thesis,JATE University,Szeged,Hungary
    Yang,Y.-L.,Liu,Q.-Y.,Zhang,Y.-L.,Wang,B.,&Lu,L.1991,Acta Astronomica Sinica,32,326
    Yang,Y.,&Liu,Q.2000,A&AS,144,457
    Yilmaz,M.,Basturk,O.,Alan,N.,et al.2009,Information Bulletin on Variable Stars,5887
    Yu,Y.-X.,Xiang,F.-Y.,&Xiao,T.-Y.2015,PASJ,67,42

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