格利泽412
天球赤道座标：
11h 05m 22.3101s，+43° 31′ 51.0404″
| 观测数据 历元 J2000 分点 J2000 | |
|---|---|
| 星座 | 大熊座 |
| Gliese 412 A | |
| 赤经 | 11h 05m 22.3101s[1] |
| 赤纬 | +43° 31′ 51.0404″[1] |
| 视星等 (V) | 8.68[2] |
| Gliese 412 B | |
| 赤经 | 11h 05m 30.8856s[3] |
| 赤纬 | +43° 31′ 17.8843″[3] |
| 视星等 (V) | 14.45[4] |
| 特性 | |
| 光谱分类 | M1.0V[2]/M6.0V[4] |
| U−B 色指数 | +1.16/—[5] |
| B−V 色指数 | +1.54[5]/2.08[6] |
| 天体测定 | |
| Gliese 412 A | |
| 径向速度 (Rv) | +64.9 ± 0.9[7] km/s |
| 自行 (μ) | 赤经：−4410.43±0.78[8] mas/yr 赤纬：942.93±0.70[8] mas/yr |
| 视差 (π) | 203.8876 ± 0.0332[9] mas |
| 距离 | 15.997 ± 0.003 ly (4.9047 ± 0.0008 pc) |
| 绝对星等 (MV) | 10.34[10] |
| Gliese 412 B | |
| 自行 (μ) | 赤经：−4339.891±0.167 mas/yr 赤纬：960.780±0.162 mas/yr |
| 视差 (π) | 203.8323 ± 0.0500[11] mas |
| 距离 | 16.001 ± 0.003 ly (4.906 ± 0.001 pc) |
| 绝对星等 (MV) | 16.05[10] |
| 详细资料 | |
| GJ 412 A | |
| 质量 | 0.48[10] M☉ |
| 半径 | 0.38[12] R☉ |
| 表面重力 (log g) | 4.90[13] |
| 温度 | 3,687[13]/ K |
| 金属量 [Fe/H] | -0.43[13] dex |
| 自转速度 (v sin i) | <3[14] km/s |
| 年龄 | 3[12] Gyr |
| GJ 412 B | |
| 质量 | 0.10[10] M☉ |
| 半径 | 0.13[12] R☉ |
| 温度 | 2,700[6] K |
| 自转速度 (v sin i) | 7.7±1.7[14] km/s |
| 其他命名 | |
| 参考资料库 | |
| SIMBAD | The system |
| A | |
| B | |
  Gliese 412 Gliese 412在大熊座的位置 | |
Gliese 412是一个位于大熊座的双星系统。[16] 距离太阳16光年。这两个组成部分都是相对暗淡的红矮星。
该系统的两个恒星组成部分的预计距离约为152天文单位，估计的轨道半长轴为190天文单位。[17] 主星大约有太阳质量的48% ，而伴星只有10%。[10] 主星的自转速度小于3公里/秒；伴星的自转速度为7.7±1.7 公里/秒。[14] 该系统的空间速度分量为 U = 141、V = –7 和 W = 7。它们是银河系成员。[14]
X 射线源[编辑]
伴星是一颗耀星，被称为 WX 大熊座。它的特征是一颗UV Ceti型变星，光度偶尔会增加。早在1939年，荷兰天文学家阿德里安·范马纳恩就观测到了这颗恒星的耀斑。[18]
伴星 (WX 大熊座)已被确定为X 射线源，而主星未检测到明显的 X 射线发射。[19] 视差为 204.059 ±0.169 mas, 代表距离太阳约为 16 光年。[3]
参考资料[编辑]
- ^ 1.0 1.1 Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365
. doi:10.1051/0004-6361/201833051. VizieR中此天体在盖亚望远镜第二批数据发布的记录
- ^ 2.0 2.1 2.2 2.3 [ BD+44 2051] 请检查
|url=值 (帮助). SIMBAD. 斯特拉斯堡天文资料中心. - ^ 3.0 3.1 3.2 Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365 . doi:10.1051/0004-6361/201833051. VizieR中此天体在盖亚望远镜第二批数据发布的记录
- ^ 4.0 4.1 4.2 [ BD+44 2051B] 请检查
|url=值 (帮助). SIMBAD. 斯特拉斯堡天文资料中心. - ^ 5.0 5.1 Nicolet, B. Photoelectric photometric Catalogue of homogeneous measurements in the UBV System. Observatory. 1978. Bibcode:1978ppch.book.....N.
- ^ 6.0 6.1 Casagrande, Luca; et al. M dwarfs: effective temperatures, radii and metallicities. Monthly Notices of the Royal Astronomical Society. September 2008, 389 (2): 585–607. Bibcode:2008MNRAS.389..585C. S2CID 14353142. arXiv:0806.2471 . doi:10.1111/j.1365-2966.2008.13573.x.
- ^ 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. June 20–24, 1966. Bibcode:1967IAUS...30...57E.
- ^ 8.0 8.1 van Leeuwen, F. Validation of the new Hipparcos reduction. Astronomy and Astrophysics. 2007, 474 (2): 653–664. Bibcode:2007A&A...474..653V . arXiv:0708.1752 . doi:10.1051/0004-6361:20078357 .Vizier catalog entry
- ^ 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. - ^ 10.0 10.1 10.2 10.3 10.4 The 100 nearest star systems. Research Consortium On Nearby Stars. 2009-09-14 [2009-09-14]. （原始内容存档于2007-11-12）.
- ^ 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. - ^ 12.0 12.1 12.2 Mann, Andrew W.; et al, How to Constrain Your M Dwarf: Measuring Effective Temperature, Bolometric Luminosity, Mass, and Radius, The Astrophysical Journal, May 2015, 804 (1): 38, Bibcode:2015ApJ...804...64M, S2CID 19269312, arXiv:1501.01635 , doi:10.1088/0004-637X/804/1/64, 64.
- ^ 13.0 13.1 13.2 Soubiran, C.; Bienaymé, O.; Mishenina, T. V.; Kovtyukh, V. V. Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants. Astronomy and Astrophysics. March 2008, 480 (1): 91–101. Bibcode:2008A&A...480...91S. S2CID 16602121. arXiv:0712.1370 . doi:10.1051/0004-6361:20078788.
- ^ 14.0 14.1 14.2 14.3 Delfosse, Xavier; Forveille, Thierry; Perrier, Christian; Mayor, Michel. Rotation and chromospheric activity in field M dwarfs. Astronomy and Astrophysics. March 1998, 331: 581–595. Bibcode:1998A&A...331..581D.
- ^ [ ** VBS 18] 请检查
|url=值 (帮助). SIMBAD. 斯特拉斯堡天文资料中心. - ^ Gould, Andrew; Chanamé, Julio. New Hipparcos-based Parallaxes for 424 Faint Stars. The Astrophysical Journal Supplement Series. February 2004, 150 (2): 455–464. Bibcode:2004ApJS..150..455G. S2CID 8494577. arXiv:astro-ph/0309001 . doi:10.1086/381147.
- ^ Reid, I. Neill; Gizis, John E. Low-Mass Binaries and the Stellar Luminosity Function. Astronomical Journal. June 1997, 113: 2246–2269. Bibcode:1997AJ....113.2246R. doi:10.1086/118436.
- ^ Joy, Alfred H. Stellar Flares. Astronomical Society of the Pacific Leaflets. June 1967, 10 (456): 41–48. Bibcode:1967ASPL...10...41J.
- ^ Schmitt JHMM; Fleming TA; Giampapa MS. The X-Ray View of the Low-Mass Stars in the Solar Neighborhood. Astrophys. J. September 1995, 450 (9): 392–400. Bibcode:1995ApJ...450..392S. doi:10.1086/176149.
参见[编辑]
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