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小犬座YZ

天球赤道座标：星图 07h 44m 40.17262s, +03° 33′ 08.8778″
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YZ Canis Minoris

小犬座YZ的光变曲线，主图显示了周期性的亮度变化和几个耀斑。插图显示了具有扩展时间尺度的最强耀斑。
观测资料
历元 J2000
星座 小犬座
星官
赤经 07h 44m 40.17230s[1]
赤纬 +03° 33′ 08.8752″[1]
视星等（V） 11.15[2]
特性
光谱分类M5 V[3]
B−V 色指数1.61[2]
天体测定
径向速度 (Rv)+26.53±0.30[4] km/s
自行 (μ) 赤经：−347.782[1] mas/yr
赤纬：−445.702[1] mas/yr
视差 (π)166.9769 ± 0.0343[1] mas
距离19.533 ± 0.004 ly
(5.989 ± 0.001 pc)
绝对星等 (MV)12.32[5]
详细资料
质量0.308[6] M☉
半径0.324[6] R☉
表面重力 (log g)5.0[7]
亮度0.012[1] L☉
温度3,125±61[8] K
金属量 [Fe/H]−0.26±0.08[8] dex
自转2.8[6] days
自转速度 (v sin i)4.0[9] km/s
年龄49[10] Myr
其他命名
YZ CMI、​BD+35°2496、​GJ 285、​HIP 37766、​SAO 63793、​G 50-4、​G 112-46、​LFT 547、​LHS 1943、​LSPM J0744+0333、​LTT 12064、​NLTT 18373、​PLX 1827、​PM 07421+0341、​Ross 882、​TYC 183-2190-1、​GSC 00183-02190、​IRAS 07420+0340、​2MASS J07444018+0333089[11]
参考数据库
SIMBAD资料
YZ Canis Minoris is located in the constellation Canis Minor
YZ Canis Minoris is located in the constellation Canis Minor
YZ
小犬座YZ在小犬座的位置

小犬座YZ 是位于小犬座中的一颗红色恒星。视星等为11.15[2]，肉眼无法看到它。目前，这颗恒星正以+26.5公里/秒的日心径向速度向更远的地方移动。[4]大约162,000年前，当它以10.2光年的距离通过近日点时，它最接近地球。[12]小犬座YZ是绘架座β移动星群的潜在成员。[13]

这是一颗红矮星，恒星分类为M5V。[3] 它也是耀星，因其恒星耀斑比太阳的耀斑更强大而得名，并且大约是木星大小的三倍。[14]

参考

  1. ^ 1.0 1.1 1.2 1.3 1.4 1.5 Vallenari, A.; et al. Gaia Data Release 3. Summary of the content and survey properties. Astronomy & Astrophysics. 2022. arXiv:2208.00211 可免费查阅. doi:10.1051/0004-6361/202243940 可免费查阅.  已忽略未知参数|collaboration= (帮助) Gaia DR3 record for this source at VizieR.
  2. ^ 2.0 2.1 2.2 Astudillo-Defru, N.; et al. Magnetic activity in the HARPS M dwarf sample. The rotation-activity relationship for very low-mass stars through R'(HK). Astronomy & Astrophysics. April 2017, 600: 15. Bibcode:2017A&A...600A..13A. S2CID 119237202. arXiv:1610.09007 可免费查阅. doi:10.1051/0004-6361/201527078. A13. 
  3. ^ 3.0 3.1 West, Andrew A.; et al. An Activity-Rotation Relationship and Kinematic Analysis of Nearby Mid-to-Late-Type M Dwarfs. The Astrophysical Journal. October 2015, 812 (1): 12. Bibcode:2015ApJ...812....3W. S2CID 17434970. arXiv:1509.01590 可免费查阅. doi:10.1088/0004-637X/812/1/3. 3. 
  4. ^ 4.0 4.1 Nidever, David L.; et al. Radial Velocities for 889 Late-Type Stars. The Astrophysical Journal Supplement Series. August 2002, 141 (2): 503–522. Bibcode:2002ApJS..141..503N. S2CID 51814894. arXiv:astro-ph/0112477 可免费查阅. doi:10.1086/340570. 
  5. ^ Anderson, E.; Francis, Ch. XHIP: An extended hipparcos compilation. Astronomy Letters. 2012, 38 (5): 331. Bibcode:2012AstL...38..331A. S2CID 119257644. arXiv:1108.4971 可免费查阅. doi:10.1134/S1063773712050015. 
  6. ^ 6.0 6.1 6.2 Newton, Elisabeth R.; et al. The Hα Emission of Nearby M Dwarfs and its Relation to Stellar Rotation. The Astrophysical Journal. January 2017, 834 (1): 13. Bibcode:2017ApJ...834...85N. S2CID 55000202. arXiv:1611.03509 可免费查阅. doi:10.3847/1538-4357/834/1/85. 85. 
  7. ^ Lépine, Sébastien; et al. A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky. The Astronomical Journal. 2013, 145 (4): 102. Bibcode:2013AJ....145..102L. S2CID 117144290. arXiv:1206.5991 可免费查阅. doi:10.1088/0004-6256/145/4/102. 
  8. ^ 8.0 8.1 Gaidos, Eric; Mann, Andrew W. M dwarf metallicities and giant planet occurrence: ironing out uncertainties and systematics. The Astrophysical Journal. August 2014, 791 (1): 9. Bibcode:2014ApJ...791...54G. S2CID 118744016. arXiv:1406.4071 可免费查阅. doi:10.1088/0004-637X/791/1/54. 54. 
  9. ^ Reiners, Ansgar; et al. The CARMENES search for exoplanets around M dwarfs. High-resolution optical and near-infrared spectroscopy of 324 survey stars. Astronomy and Astrophysics. 2018, 612: A49. Bibcode:2018A&A...612A..49R. S2CID 62818673. arXiv:1711.06576 可免费查阅. doi:10.1051/0004-6361/201732054. 
  10. ^ Meshkat, Tiffany; et al. A Direct Imaging Survey of Spitzer-detected Debris Disks: Occurrence of Giant Planets in Dusty Systems. The Astronomical Journal. December 2017, 154 (6): 21. Bibcode:2017AJ....154..245M. S2CID 42042014. arXiv:1710.04185 可免费查阅. doi:10.3847/1538-3881/aa8e9a. 245. 
  11. ^ YZ CMi. SIMBAD. 斯特拉斯堡天文资料中心. 
  12. ^ Bailer-Jones, C. A. L. Close encounters of the stellar kind. Astronomy & Astrophysics. March 2015, 575: 13. Bibcode:2015A&A...575A..35B. S2CID 59039482. arXiv:1412.3648 可免费查阅. doi:10.1051/0004-6361/201425221. A35. 
  13. ^ Nakajima, Tadashi; Morino, Jun-Ichi. Potential Members of Stellar Kinematic Groups within 30 pc of the Sun. The Astronomical Journal. January 2012, 143 (1): 2. Bibcode:2012AJ....143....2N. doi:10.1088/0004-6256/143/1/2 可免费查阅. 
  14. ^ First flares on a distant star. New Scientist. February 4, 1982: 305. 
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