List of star systems within 30–35 light-years

This is a list of star systems within 30-35 light years of Earth.

Star system Median distance (ly) Stars in system Spectral type Apparent magnitude (V) Comments and references
Gamma Pavonis 30.1 ± 0.2 1 F9V 4.22 [1][2]
HD 102365 30.1 ± 0.2 2 G2V + M4V 4.88 + 15 has 1 known planet[2][3][4][5]
2MASS 1750-00 30.1 ± 0.7 1 L
Gliese 176 30.7 ± 0.7 1 M2V 9.95 has 1 known planet[6]
2MASS J11592743-5247188 30.9 ± 0.04 1 M9V [7]Brown Dwarf
2MASS 0034+0523 30.9 +2.4
-2.1 		1 T
LHS 194 31.0 ± 0.8 1 DQ
61 Ursae Majoris 31.1 ± 0.2 1 G8V 5.35 [8][9]
HR 4458 31.1 ± 0.2 2 K0V + DC8 5.97 + 15 [2][10][11]
BPS CS 22898-0066 31.2 ± 7.1 1 MV
2MASS J11553952-3727350 31.2 ± 1.5 1 L
TYC 3251-1875-1 31.5 ± 5.9 1 MV
WISE J140533.32+835030.5 31.6 ± 5.5 1 L
CFBD J0059-01 31.6 ± 0.6 1 T
LHS 145 31.7 ± 0.3 1 DA
Gliese 638 31.9 ± 0.3 1 K7V 8.11 [9]
12 Ophiuchi 31.9 ± 0.3 1 K2V 5.77 [12]
LP 655-48 32.0 ± 3.6 1 MV
WISE 0811-8051 32.0 1 T9.5
2MASS J2139+0220 32.1 ± 0.6 1 T
AU Microscopii 32.3 ± 0.3 3 M1Ve 8.73 [13]
HR 511 32.5 ± 0.2 1 K0V 5.63 [10][14]
WISE 1614+1739 32.6 1 T9 19.08
ULAS 1335+11 32.6 ± 0.5 1 T
Gliese 22 32.8 ± 0.7 3 M2.5Ve + M3V 10.29 + 12.19 + 13.2
WISE 1150+6302 32.9 1 T8 17.72
WISE 1318-1758 32.9 1 T9
WISE 1217+1626 32.9 +6.4
-4.6 		2 T9 17.83
HR 5256 33.0 ± 0.2 1 K3V 6.520 [15][16]
Alpha Mensae 33.1 ± 0.2 1 G7V 5.09 [2][10]
Gliese 453 33.2 ± 0.3 1 KV
Gliese 436 33.4 ± 0.8 1 M2.5V 10.67 has 1 known planet[17]
Gliese 127.1 33.4 ± 0.6 2 DA3.0 [18]
Gliese 3182 33.6 ± 1.3 1 DAZ9 [19]
Pollux 33.7 ± 0.3 1 K0III 1.14 has 1 known planet[20][21][22]
Gliese 649 33.7 ± 0.5 1 M1.5V 9.62 has 1 known planet[23]
Gliese 339.1 33.7 ± 0.6 1 DC7P
2MASS 0559-1404 33.76 ± 0.35 1 T
HD 17925 33.9 ± 0.3 1 K1V 6.04 [10][24]
2MASS 1237+6526 33.9 ± 1.8 1 T6.5V 16.15 [25]
WISE 1322-2340 33.9 1 T8 17.01
WISE J2030+0749 34.2 ± 8.5 1 T1.5 [26]
Iota Persei 34.4 ± 0.3 1 G0V 4.05
2MASS 1047+2124 34.4 ± 1.4 1 T
2MASS J00501994−3322402 34.5 ± 0.9 1 T
WD 0821-669 34.7 ± 0.4 1 DA9
2MASS 2228-4310 34.7 +2.8
-2.4 		1 T
Zeta Herculis 34.8 ± 0.2 2 F9IV + G7V 2.81 [27][28]
Gliese 617 34.8 ± 0.4 2 MV
2MASS J08251968+2115521 34.8 ± 0.4 1 L
2MASS 0243-2453 34.8 ± 1.4 1 T6 [25]
HD 160346 34.9 ± 0.5 1 KV
WISE 0734-7157 34.9 1 Y0 20.41 [29]

See also

References

  1. ↑ Jehin, E.; et al. (January 1999), "Abundance correlations in mildly metal-poor stars", Astronomy and Astrophysics, 341: 241–255, arXiv:astro-ph/9809405Freely accessible, Bibcode:1999A&A...341..241J
  2. 1 2 3 4 Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv:astro-ph/0603770Freely accessible, Bibcode:2006AJ....132..161G, doi:10.1086/504637
  3. ↑ Poveda, A.; et al. (April 1994), "Statistical studies of visual double and multiple stars. II. A catalogue of nearby wide binary and multiple systems", Revista Mexicana de Astronomía y Astrofísica, 28 (1): 43–89, Bibcode:1994RMxAA..28...43P
  4. ↑ Feinstein, A. (1966), "Photoelectric observations of Southern late-type stars", The Information Bulletin for the Southern Hemisphere, 8: 30, Bibcode:1966IBSH....8...30F
  5. ↑ Raghavan, Deepak; et al. (September 2010), "A Survey of Stellar Families: Multiplicity of Solar-type Stars", The Astrophysical Journal Supplement, 190 (1): 1–42, arXiv:1007.0414Freely accessible, Bibcode:2010ApJS..190....1R, doi:10.1088/0067-0049/190/1/1 For the adopted physical separation, see Table 11 in the appendix.
  6. ↑ Forveille, T.; et al. (January 2009). "The HARPS search for southern extra-solar planets. XIV. Gl 176b, a super-Earth rather than a Neptune, and at a different period". Astronomy and Astrophysics. 493 (2): 645–650. arXiv:0809.0750Freely accessible. Bibcode:2009A&A...493..645F. doi:10.1051/0004-6361:200810557.
  7. ↑ http://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J11592743-5247188
  8. ↑ Cornide, M.; Rego, M. (October 1984). "Iron abundances in G dwarfs". Astrophysics and Space Science. 105 (1): 55–65. Bibcode:1984Ap&SS.105...55C. doi:10.1007/BF00651207.
  9. 1 2 Wilson, O. C. (November 1962). "Relationship Between Colors and Spectra of Late Main-Sequence Stars". Astrophysical Journal. 136: 793. Bibcode:1962ApJ...136..793W. doi:10.1086/147437.
  10. 1 2 3 4 Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV data. Bibcode:1986EgUBV........0M.
  11. ↑ Holberg, J. B.; et al. (November 2013). "Where are all the Sirius-like binary systems?". Monthly Notices of the Royal Astronomical Society. 435 (3): 2077–2091. arXiv:1307.8047Freely accessible. Bibcode:2013MNRAS.435.2077H. doi:10.1093/mnras/stt1433.
  12. ↑ Fuhrmann, Klaus (February 2008), "Nearby stars of the Galactic disc and halo - IV", Monthly Notices of the Royal Astronomical Society, 384 (1): 173–224, Bibcode:2008MNRAS.384..173F, doi:10.1111/j.1365-2966.2007.12671.x
  13. ↑ Torres, C. A. O.; et al. (December 2006), "Search for associations containing young stars (SACY). I. Sample and searching method", Astronomy and Astrophysics, 460 (3): 695–708, arXiv:astro-ph/0609258Freely accessible, Bibcode:2006A&A...460..695T, doi:10.1051/0004-6361:20065602
  14. ↑ White, Russel J.; Gabor, Jared M.; Hillenbrand, Lynne A. (June 2007), "High-Dispersion Optical Spectra of Nearby Stars Younger Than the Sun", The Astronomical Journal, 133 (6): 2524–2536, arXiv:0706.0542Freely accessible, Bibcode:2007AJ....133.2524W, doi:10.1086/514336.
  15. ↑ Oja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI". Astronomy and Astrophysics Supplement Series. 89 (2): 415–419. Bibcode:1991A&AS...89..415O.
  16. ↑ Marrese, P. M.; Boschi, F.; Munari, U. (August 2003). "High resolution spectroscopy over lambda lambda 8500-8750 Å for GAIA. IV. Extending the cool MK stars sample". Astronomy and Astrophysics. 406: 995–999. Bibcode:2003A&A...406..995M. doi:10.1051/0004-6361:20030647.
  17. ↑ Butler, R. Paul; et al. (2004). "A Neptune-Mass Planet Orbiting the Nearby M Dwarf GJ 436". The Astrophysical Journal. 617 (1): 580–588. arXiv:astro-ph/0408587Freely accessible. Bibcode:2004ApJ...617..580B. doi:10.1086/425173. Retrieved 2009-12-26.
  18. ↑ http://simbad.u-strasbg.fr/simbad/sim-id?Ident=LB+3303
  19. ↑ http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Gliese++3182
  20. ↑ Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237: 0. Bibcode:2002yCat.2237....0D.
  21. ↑ Morgan, W. W.; Keenan, P. C. (1973), "Spectral Classification", Annual Review of Astronomy and Astrophysics, 11: 29, Bibcode:1973ARA&A..11...29M, doi:10.1146/annurev.aa.11.090173.000333
  22. ↑ Hatzes, A. P.; et al. (2006), "Confirmation of the planet hypothesis for the long-period radial velocity variations of β Geminorum", Astronomy and Astrophysics, 457: 335–341, arXiv:astro-ph/0606517Freely accessible, Bibcode:2006A&A...457..335H, doi:10.1051/0004-6361:20065445
  23. ↑ Johnson, John Asher; et al. (2010). "The California Planet Survey II. A Saturn-Mass Planet Orbiting the M Dwarf Gl649". The Publications of the Astronomical Society of the Pacific. 122 (888): 149–155. arXiv:0912.2730Freely accessible. Bibcode:2010PASP..122..149J. doi:10.1086/651007.
  24. ↑ Montes, D.; et al. (2001), "Late-type members of young stellar kinematic groups - I. Single stars", Monthly Notices of the Royal Astronomical Society, 328 (1): 45–63, arXiv:astro-ph/0106537Freely accessible, Bibcode:2001MNRAS.328...45M, doi:10.1046/j.1365-8711.2001.04781.x.
  25. 1 2 Vrba, F. J.; Henden, A. A.; Luginbuhl, C. B.; Guetter, H. H.; Munn, J. A.; Canzian, B.; Burgasser, A. J.; Kirkpatrick, J. Davy; Fan, X.; Geballe, T. R.; Golimowski, D. A.; Knapp, G. R.; Leggett, S. K.; Schneider, D. P.; Brinkman, J. (2004). "Preliminary Parallaxes of 40 L and T Dwarfs from the U.S. Naval Observatory Infrared Astrometry Program". arXiv:astro-ph/0402272Freely accessible.
  26. ↑ Bihain, Gabriel; Scholz, Ralf-Dieter; Storm, Jesper; Schnurr, Olivier (2013). "An overlooked brown dwarf neighbour (T7.5 at d~5pc) of the Sun and two additional T dwarfs at about 10pc". arXiv:1307.2722Freely accessible.
  27. ↑ Edwards, T. W. (April 1976), "MK classification for visual binary components", Astronomical Journal, 81: 245–249, Bibcode:1976AJ.....81..245E, doi:10.1086/111879
  28. ↑ Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99), Bibcode:1966CoLPL...4...99J
  29. ↑ Kirkpatrick, J. D.; Gelino, C. R.; Cushing, M. C.; Mace, G. N.; Griffith, R. L.; Skrutskie, M. F.; Marsh, K. A.; Wright, E. L.; Eisenhardt, P. R.; McLean, I. S.; Mainzer, A. K.; Burgasser, A. J.; Tinney, C. G.; Parker, S.; Salter, G. (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal. 753 (2): 156. arXiv:1205.2122Freely accessible. Bibcode:2012ApJ...753..156K. doi:10.1088/0004-637X/753/2/156.
This article is issued from Wikipedia - version of the 11/13/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.