金牛座EQ是黄道星座金牛座的一颗三合星,它包括密接的食双星。该系统过于黯淡,无法用肉眼观察,基线的视星等为10.5等[3]。在食的期间,系统的主极小期亮度降至11.03等,然后在次极小期降至10.97等[3]。次极小期是全食[7]。根据视差的量测,它位于距离太阳约730光年的地方[2]。
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恒星HV 6189在1940年被哈罗·沙普利( Harlow Shapley)和艾米莉·M·休斯( Emily M. Hughes)确认为短周期变星[9],然后再1954年,苏联天文学家弗拉基米尔·普拉托诺维奇·采谢维奇对其进行了更深入的研究[6]。它被确定为大熊座W型变星,并被注意到位于疏散星团昴宿星团的区域[10]。对采谢维奇数据的分析以及B.S.Whitney在1972年的后续观测表明,它的周期是可变的。他在孔科利天文台的观测显示周期为8.19 h[11]。Wystan Benbow和Robert L.Mutel在1995年建立了食变星的光变曲线,显示了恒星表面存在活动区的证据[12]。轨道周期的变化继续被观察到,在2002年Theodor Pribulla和Martin Vańko提出它是由系统中的第三个天体引起的。他们将其建模为低质量的红矮星,轨道周期为50.2年[13]。
这是一个浅接触的联星系统[7],属于大熊座W型变星的A子型[3]。它的轨道周期为8.1924小时[6],半长轴是太阳半径的2.48倍。轨道呈现周期性变化,其周期为22.7年,振幅为0.0058天。2010年观测到类似凌的事件[7]。质量更大的成分是一颗有很深对流层的太阳型恒星,出现磁活动,覆盖着显著的星斑 [4]。
Shapley, Harlow; Hughes, Emily M., Variable stars in high galactic latitudes, Annals of the Astronomical Observatory of Harvard College, 1940, 90 (4): 163–175, Bibcode:1940AnHar..90..163S.
Artiukhina, N. M., Proper Motions of three W UMa Type Stars in the Pleiades Region, Peremennye Zvezdy, 1961, 13: 366, Bibcode:1961PZ.....13..366A (俄语).
Whitney, B. S., The Period of EQ Tauri, Information Bulletin on Variable Stars, February 1972, 633 (1): 1, Bibcode:1972IBVS..633....1W.
Benbow, W. R.; Mutel, R. L., Eclipse Observations of EQ Tau, Information Bulletin on Variable Stars, May 1995, 4187 (1): 1, Bibcode:1995IBVS.4187....1B.
Pribulla, T.; Vanko, M., Photoelectric photometry of eclipsing contact binaries: U Peg, YY CrB, OU Ser and EQ Tau, Contributions of the Astronomical Observatory Skalnate Pleso, April 2002, 32 (1): 79–98, Bibcode:2002CoSka..32...79P.
- Tvardovskyi, D. E., Third components with elliptical orbits in the eclipsing binaries: EQ Tau, IR Cas, IV Cas, RY Aqr & RZ Com, Annales Astronomiae Novae, January 2020, 1: 231–238, Bibcode:2020AANv....1..231T, arXiv:1912.12639 .
- Hasanzadeh, A.; et al, New light curve analysis and period changes of the overcontact binary EQ Tauri, New Astronomy, January 2015, 34: 262–265, Bibcode:2015NewA...34..262H, doi:10.1016/j.newast.2014.07.013.
- Elkhateeb, M. M.; Nouh, M. I., A holistic study of the eclipsing binary EQ Tau (PDF), Journal of Physics and Astronomy Research, 2014, 1 (3): 15 [2022-03-13], arXiv:1406.1661 .[失效链接]
- Alton, K. B., A Multi-year Multi-passband CCD Photometric Study of the W UMa Binary EQ Tauri, The Journal of the American Association of Variable Star Observers, December 2009, 37 (2): 148, Bibcode:2009JAVSO..37..148A.
- Hrivnak, Bruce J.; Lu, Wenxian; Eaton, Jeffery; Kenning, Daniel, Light-Curve Study and Physical Properties of the Contact Binary EQ Tauri, The Astronomical Journal, August 2006, 132 (2): 960–966, Bibcode:2006AJ....132..960H, S2CID 120523899, doi:10.1086/505691 .
- Alton, Kevin B., A Backyard CCD Photometric Study of the Neglected W UMa Binary EQ Tauri, Open European Journal on Variable Stars, June 2006, 39: 1, Bibcode:2006OEJV...39....1A.
- Vaňko, M.; et al, New Parameters of the Contact Binary Systems YY CRB and EQ Tau, Baltic Astronomy, 2004, 13: 151–155, Bibcode:2004BaltA..13..151V.
- Yang, Yulan; Liu, Qingyao, A Photometric Study of the Contact Binary EQ Tauri, The Astronomical Journal, December 2002, 124 (6): 3358–3363, Bibcode:2002AJ....124.3358Y, S2CID 123447240, doi:10.1086/344763 .
- Qian, Shengbang; Ma, Yuan, Period Studies of Some Neglected Close Binaries: EP Andromedae, V724 Aquilae, SS Comae, AM Eridani, FZ Orionis, BY Pegasi, EQ Tauri, and NO Vulpeculae, The Publications of the Astronomical Society of the Pacific, June 2001, 113 (784): 754–763, Bibcode:2001PASP..113..754Q, S2CID 121169370, doi:10.1086/320808 .
- Buckner, M.; et al, Eclipse Timing Observations of Three Close Binaries, Information Bulletin on Variable Stars, February 1998, 4559 (1): 1, Bibcode:1998IBVS.4559....1B.