Tham khảo BD Phoenicis

  1. ↑ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
  2. 1 2 3 4 Koen, C.; Paunzen, E.; Van Wyk, F.; Marang, F.; Chernyshova, I. V.; Andrievsky, S. M. (2003). "The pulsational characteristics of the λ Bootis type star BD Phe (HD 11413)". Monthly Notices of the Royal Astronomical Society. 338 (4): 931. Bibcode:2003MNRAS.338..931K.
  3. ↑ Samus', N. N; Kazarovets, E. V; Durlevich, O. V; Kireeva, N. N; Pastukhova, E. N (2017), "General catalogue of variable stars: Version GCVS 5.1", Astronomy Reports, 61 (1): 80, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085.
  4. ↑ Gray, R. O.; Garrison, R. F. (1987). "The Early A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation". The Astrophysical Journal Supplement Series. 65: 581. Bibcode:1987ApJS...65..581G.
  5. 1 2 3 Draper, Z. H.; Matthews, B. C.; Kennedy, G. M.; Wyatt, M. C.; Venn, K. A.; Sibthorpe, B. (2016). "IR excesses around nearby Lambda Boo stars are caused by debris discs rather than ISM bow waves". Monthly Notices of the Royal Astronomical Society. 456 (1): 459. Bibcode:2016MNRAS.456..459D.
  6. ↑ Faraggiana, R.; Bonifacio, P.; Caffau, E.; Gerbaldi, M.; Nonino, M. (2004). "λ Bootis stars with composite spectra". Astronomy and Astrophysics. 425 (2): 615–626. arXiv:astro-ph/0406265. Bibcode:2004A&A...425..615F. doi:10.1051/0004-6361:20040216.
  7. Gontcharov, G. A. (tháng 11 năm 2006), “Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system”, Astronomy Letters 32 (11): 759–771, Bibcode:2006AstL...32..759G, arXiv:1606.08053, doi:10.1134/S1063773706110065. 
  8. “BD Phe”. SIMBAD. Centre de données astronomiques de Strasbourg. 

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