Tham khảo Lambda Serpentis

  1. 1 2 3 4 5 6 van Leeuwen, F. (2007). “Validation of the new Hipparcos reduction”. Astronomy and Astrophysics 474 (2): 653–664. Bibcode:2007A&A...474..653V. arXiv:0708.1752. doi:10.1051/0004-6361:20078357.  Mục từ trong danh lục Vizier
  2. 1 2 3 4 Johnson, H. L.; Morgan, W. W. (1953). “Fundamental stellar photometry for standards of spectral type on the revised system of the Yerkes spectral atlas”. Astrophysical Journal 117: 313–352. Bibcode:1953ApJ...117..313J. doi:10.1086/145697. 
  3. 1 2 3 “lam Ser -- Spectroscopic binary”. SIMBAD. Centre de Données astronomiques de Strasbourg. Truy cập ngày 15 tháng 12 năm 2010. 
  4. 1 2 Wilson, Ralph Elmer (1953). “General Catalogue of Stellar Radial Velocities”. Carnegie Institute Washington D.C. Publication (Washington: Carnegie Institution of Washington). Bibcode:1953GCRV..C......0W. 
  5. ↑ Holmberg, J.; Nordström, B.; Andersen, J. (tháng 7 năm 2009), “The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics”, Astronomy and Astrophysics 501 (3): 941–947, Bibcode:2009A&A...501..941H, arXiv:0811.3982, doi:10.1051/0004-6361/200811191. 
  6. 1 2 Valenti, J. A.; Fishcer, D. A. (2005). “Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs”. Astrophysical Journal Supplement Series 159 (1): 141–166. Bibcode:2005ApJS..159..141V. doi:10.1086/430500. 
  7. ↑ van Belle, Gerard T.; von Braun, Kaspar (2009). “Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars”. The Astrophysical Journal 694 (2): 1085–1098. Bibcode:2009ApJ...694.1085V. arXiv:0901.1206. doi:10.1088/0004-637X/694/2/1085. 
  8. 1 2 Fuhrmann, Klaus (tháng 10 năm 1998). “Nearby stars of the Galactic disk and halo”. Astronomy and Astrophysics 338: 161–183. Bibcode:1998A&A...338..161F. 
  9. 1 2 Kovtyukh; Soubiran, C.; Belik, S. I.; Gorlova, N. I. (2003). “High precision effective temperatures for 181 F-K dwarfs from line-depth ratios”. Astronomy and Astrophysics 411 (3): 559–564. Bibcode:2003A&A...411..559K. arXiv:astro-ph/0308429. doi:10.1051/0004-6361:20031378. 
  10. ↑ Bernacca P. L.; Perinotto M. (1970). “A catalogue of stellar rotational velocities”. Contributi Osservatorio Astronomico di Padova in Asiago 239 (1): 1. Bibcode:1970CoAsi.239....1B. 
  11. ↑ Mamajek, Eric E.; Hillenbrand, Lynne A. (tháng 11 năm 2008). “Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics”. The Astrophysical Journal 687 (2): 1264–1293. Bibcode:2008ApJ...687.1264M. arXiv:0807.1686. doi:10.1086/591785. 
  12. ↑ Dybczyński, P. A. (tháng 4 năm 2006), “Simulating observable comets. III. Real stellar perturbers of the Oort cloud and their output”, Astronomy and Astrophysics 449 (3): 1233–1242, Bibcode:2006A&A...449.1233D, doi:10.1051/0004-6361:20054284 
  13. 1 2 Morbey, C. L.; Griffith R. F. (1987). “On the reality of certain spectroscopic orbits”. Astrophysical Journal 317 (1): 343–352. Bibcode:1987ApJ...317..343M. doi:10.1086/165281. 

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Tài liệu tham khảo

WikiPedia: Lambda Serpentis http://adsabs.harvard.edu/abs/1953ApJ...117..313J http://adsabs.harvard.edu/abs/1953GCRV..C......0W http://adsabs.harvard.edu/abs/1970CoAsi.239....1B http://adsabs.harvard.edu/abs/1987ApJ...317..343M http://adsabs.harvard.edu/abs/1998A&A...338..161F http://adsabs.harvard.edu/abs/2003A&A...411..559K http://adsabs.harvard.edu/abs/2005ApJS..159..141V http://adsabs.harvard.edu/abs/2006A&A...449.1233D http://adsabs.harvard.edu/abs/2006AJ....132..177W http://adsabs.harvard.edu/abs/2007A&A...474..653V