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狮子座AD

狮子座AD(Gliese 388)是一颗位于狮子座红矮星。距离太阳大约有16光年。狮子座AD是一颗光谱分类为M3.5V的主序星。 [4]它是一颗亮度随机增加的耀星。[5][14]

AD Leonis

狮子座AD上耀斑的U、B、V 和 R光变曲线[1]
观测资料
历元 J2000
星座 狮子座
星官
赤经 10h 19m 36.277s[2]
赤纬 +19° 52′ 12.06″[2]
视星等（V） 9.32[3]
特性
光谱分类M3.5eV[4]
U−B 色指数+1.06[3]
B−V 色指数+1.54[3]
变星类型耀星[5]
天体测定
径向速度 (Rv)+10.8[6] km/s
自行 (μ) 赤经：–501.8[2] mas/yr
赤纬：–42.8[2] mas/yr
视差 (π)201.4064 ± 0.0296[7] mas
距离16.194 ± 0.002 ly
(4.9651 ± 0.0007 pc)
绝对星等 (MV)10.87[8]
详细资料
质量0.39–0.42[8][9] M☉
半径0.39[9] R☉
表面重力 (log g)4.79[10]
亮度0.024[10] L☉
温度3,390 ± 19[11] K
金属量 [Fe/H]+0.28 ± 0.17[11] dex
自转速度 (v sin i)3[9][12] km/s
年龄25-300[13] Myr
其他命名
Gliese 388, BD+20 2465, G 54-23, LHS 5167, LTT 12761, NLTT 24015, SAO 81292, PLX 2420, TYC 1423-174-1[14]
参考资料库
SIMBAD资料
AD Leonis is located in the constellation Leo.
AD Leonis is located in the constellation Leo.
AD Leonis
狮子座AD在狮子座的位置

特性

狮子座AD是一颗M型星，光谱类型为M3.5eV，表明它是一颗主序星。它的视星等为9.43。[8][10] 它大约有太阳质量的39–42%——高于恒星完全对流的质量[15] — 和太阳半径的39%。[8][9]这颗恒星的预计自转速度仅为3 公里/秒，[12]但它每 2.24 天完成一次自转。[15]它是一颗相对年轻的恒星，估计年龄为25亿年，[13]并被认为是年轻盘星族的一员。[16]

1943年麦考密克天文台的自行研究中，它被怀疑有伴星。然而，1968 年的一项研究未能证实这一结果。[17] 1997年使用近红外散斑干涉仪进行的搜索未能检测到一颗距离恒星1-10个天文单位的伴星。[18]2001年，光学日冕仪被用来对这颗恒星进行示例，但没有发现伴星。[19]它的径向速度没有变化的迹象，表明存在看不见的伴星。[10]

这颗恒星以0.028的离心率绕银河系运行。这使得恒星距离银心近8.442kpc，远至8.926kpc。轨道倾角将它带到距银河系平面0.121 kpc远的地方。[20]

2021年，XMM-Newton在 X 射线和TESS在光学上同时观测到狮子座AD上的超级耀斑。[21]

参见

参考资料

  1. ^ Hawley, Suzanne L.; Pettersen, Bjorn R. The Great Flare of 1985 April 12 on AD Leonis. The Astrophysical Journal. September 1991, 378: 725 [17 January 2022]. Bibcode:1991ApJ...378..725H. doi:10.1086/170474. （原始内容存档于2023-03-20）. 
  2. ^ 2.0 2.1 2.2 2.3 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; et al. The Tycho-2 catalogue of the 2.5 million brightest stars. Astronomy and Astrophysics. March 2000, 355: L27–L30. Bibcode:2000A&A...355L..27H. doi:10.1888/0333750888/2862. 
  3. ^ 3.0 3.1 3.2 Nicolet, B. Catalogue of homogeneous data in the UBV photoelectric photometric system. Astronomy and Astrophysics Supplement Series. October 1978, 34: 1–49. Bibcode:1978A&AS...34....1N. 
  4. ^ 4.0 4.1 Shkolnik, Evgenya; Liu, Michael C.; Reid, I. Neill. Identifying the young low-mass stars within 25 pc. I. Spectroscopic observations. The Astrophysical Journal. July 2009, 699 (1): 649–666. Bibcode:2009ApJ...699..649S. S2CID 118623086. arXiv:0904.3323  . doi:10.1088/0004-637X/699/1/649. 
  5. ^ 5.0 5.1 Kukarkin, B. V.; Kholopov, P. N.; Pskovsky, Y. P.; Efremov, Y. N.; Kukarkina, N. P.; Kurochkin, N. E.; Medvedeva, G. I. The third edition, containing information on 20,437 variable stars discovered and designated till 1968. General Catalogue of Variable Stars 3rd. 1971. Bibcode:1971GCVS3.C......0K. 
  6. ^ Evans, D. S. The revision of the General Catalogue of Radial Velocities. Batten, Alan Henry; Heard, John Frederick (编). Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. University of Toronto: International Astronomical Union. 20–24 June 1966. Bibcode:1967IAUS...30...57E. 
  7. ^ Brown, A. G. A.; et al. Gaia Early Data Release 3: Summary of the contents and survey properties. Astronomy & Astrophysics. 2021, 649: A1. Bibcode:2021A&A...649A...1G. S2CID 227254300. arXiv:2012.01533  . doi:10.1051/0004-6361/202039657  .  已忽略未知参数|collaboration= (帮助) (勘误: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  8. ^ 8.0 8.1 8.2 8.3 The One Hundred Nearest Star Systems. Georgia State University. 1 January 2009 [2009-09-25]. （原始内容存档于2007-11-12）.  已忽略未知参数|collaboration= (帮助)
  9. ^ 9.0 9.1 9.2 9.3 Reiners, Ansgar; Basri, Gibor; Browning, Matthew. Evidence for magnetic flux saturation in rapidly rotating M stars (PDF). The Astrophysical Journal. February 2009, 692 (1): 538–545 [2021-09-11]. Bibcode:2009ApJ...692..538R. S2CID 15833388. arXiv:0810.5139  . doi:10.1088/0004-637X/692/1/538. hdl:10871/10302. （原始内容存档 (PDF)于2021-09-11）. 
  10. ^ 10.0 10.1 10.2 10.3 Pettersen, B. R.; Coleman, L. A. Chromospheric lines in red dwarf flare stars, I - AD Leonis and GX Andromedae. Astrophysical Journal. December 1981, 251 (12): 571–82. Bibcode:1981ApJ...251..571P. doi:10.1086/159500. 
  11. ^ 11.0 11.1 Rojas-Ayala, Bárbara; Covey, Kevin R.; Muirhead, Philip S.; Lloyd, James P. Metallicity and temperature indicators in M dwarf K band spectra: Testing new and updated calibrations with observations of 133 Solar neighborhood M dwarfs. The Astrophysical Journal. April 2012, 748 (2): 93. Bibcode:2012ApJ...748...93R. S2CID 41902340. arXiv:1112.4567  . doi:10.1088/0004-637X/748/2/93. 
  12. ^ 12.0 12.1 Reiners, Ansgar. The narrowest M dwarf line profiles and the rotation-activity connection at very slow rotation. Astronomy and Astrophysics. May 2007, 467 (1): 259–268. Bibcode:2007A&A...467..259R. S2CID 8672566. arXiv:astro-ph/0702634  . doi:10.1051/0004-6361:20066991. 
  13. ^ 13.0 13.1 Shkolnik, Evgenya; Liu, Michael C.; Reid, I. Neill. Identifying the young low-mass stars within 25 pc. I. Spectroscopic observations. The Astrophysical Journal. July 2009, 699 (1): 649–666. Bibcode:2009ApJ...699..649S. S2CID 118623086. arXiv:0904.3323  . doi:10.1088/0004-637X/699/1/649. 
  14. ^ 14.0 14.1 V* AD Leo – Flare Star. SIMBAD. Centre de Données astronomiques de Strasbourg. [2009-09-25]. （原始内容存档于2023-03-21）. 
  15. ^ 15.0 15.1 Reiners, Ansgar; Basri, Gibor. On the magnetic topology of partially and fully convective stars. Astronomy and Astrophysics. March 2009, 496 (3): 787–790. Bibcode:2009A&A...496..787R. S2CID 15159121. arXiv:0901.1659  . doi:10.1051/0004-6361:200811450. 
  16. ^ Sciortino, S.; Maggio, A.; Favata, F.; Orlando, S. X-ray spectroscopy of the active dM stars: AD Leo and EV Lac. Astronomy & Astrophysics. February 1999, 342 (2): 502–14. Bibcode:1999A&A...342..502S. 
  17. ^ Lippincott, S. L. Astrometric study of BD+20 2465 from photographs taken with the Sproul 24 inch refractor. Astronomical Journal. March 1969, 74: 224–228. Bibcode:1969AJ.....74..224L. doi:10.1086/110795. 
  18. ^ Oppenheimer, B. R.; Golimowski, D. A.; Kulkarni, S. R.; Matthews, K.; Nakajima, T.; Creech-Eakman, M.; Durrance, S.T. A coronagraphic survey for companions of stars within 8 parsecs. The Astronomical Journal. April 2001, 121 (4): 2189–2211. Bibcode:2001AJ....121.2189O. S2CID 119092593. arXiv:astro-ph/0101320  . doi:10.1086/319941. 
  19. ^ Leinert, C.; Henry, T.; Glindemann, A.; McCarthy, D. W., Jr. A search for companions to nearby southern M dwarfs with near-infrared speckle interferometry. Astronomy and Astrophysics. September 1997, 325: 159–166. Bibcode:1997A&A...325..159L. 
  20. ^ Allen, C.; Herrera, M. A. The galactic orbits of nearby UV Ceti stars. Revista Mexicana de Astronomía y Astrofísica. April 1998, 34: 37–46. Bibcode:1998RMxAA..34...37A. 
  21. ^ Stelzer, B.; Caramazza, M.; Raetz, St.; Argiroffi, C.; Coffaro, M. The Great Flare of 2021 November 19 on AD Leo. Simultaneous XMM-Newton and TESS observations. Solar and Stellar Astrophysics. 2022. S2CID 252199896. arXiv:2209.05068  . doi:10.1051/0004-6361/202244642. 

外部链接

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