Jump to content

Sigma Leonis

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Bibcode Bot (talk | contribs) at 03:28, 24 August 2012 (Adding 1 arxiv eprint(s), 0 bibcode(s) and 0 doi(s). Did it miss something? Report bugs, errors, and suggestions at User talk:Bibcode Bot). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Sigma Leonis
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 11h 21m 08.1943s[1]
Declination +06° 01′ 45.558″[1]
Apparent magnitude (V) 4.044[2]
Characteristics
Spectral type B9.5Vs[2]
U−B color index –0.12[3]
B−V color index –0.06[3]
Astrometry
Radial velocity (Rv)–5.3[4] km/s
Proper motion (μ) RA: –91.76[1] mas/yr
Dec.: –12.83[1] mas/yr
Parallax (π)15.24 ± 0.81 mas[1]
Distance210 ± 10 ly
(66 ± 3 pc)
Details
Radius3.3[5] R
Surface gravity (log g)3.83 ± 0.03[6] cgs
Temperature10,250[5] K
Metallicity [Fe/H]+0.0[5] dex
Rotational velocity (v sin i)70[7] km/s
Other designations
77 Leo, HR 4386, BD+06 2437, HD 98664, SAO 118804, FK5 427, HIP 55434.[2]

Sigma Leonis (σ Leo) is a blue-white 4th-magnitude star in the constellation Leo.

Sigma Leonis is of the spectral class B9.5Vs and has an apparent magnitude of +4.04.

References

  1. ^ a b c d e Perryman, M. A. C. (1997). "The HIPPARCOS Catalogue". Astronomy & Astrophysics. 323: L49 – L52. Bibcode:1997A&A...323L..49P. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |month= ignored (help)
  2. ^ a b c "sig Leo -- Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2010-06-23.
  3. ^ a b Johnson, H. L.; Iriarte, B.; Mitchell, R. I.; Wisniewskj, W. Z. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4 (99). Bibcode:1966CoLPL...4...99J.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  4. ^ Wilson, Ralph Elmer (1953). General Catalogue of Stellar Radial Velocities. Washington: Carnegie Institution of Washington. Bibcode:1953QB901.W495.....
  5. ^ a b c Lipski, Ł.; Stȩpień, K. (2008). "Effective temperatures of magnetic chemically peculiar stars from full spectral energy distributions". Monthly Notices of the Royal Astronomical Society. 385 (1): 481–492. arXiv:0712.3664. Bibcode:2008MNRAS.385..481L. doi:10.1111/j.1365-2966.2008.12856.x. {{cite journal}}: Unknown parameter |month= ignored (help)CS1 maint: multiple names: authors list (link)
  6. ^ Fitzpatrick, E. L.; Massa, D. (2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry", The Astronomical Journal, 129 (3): 1642–1662, arXiv:astro-ph/0412542, Bibcode:2005AJ....129.1642F, doi:10.1086/427855 {{citation}}: Unknown parameter |month= ignored (help)
  7. ^ Bernacca, P. L.; Perinotto, M. (1970). "A catalogue of stellar rotational velocities". Contributi Osservatorio Astronomico di Padova in Asiago. 239 (1). Bibcode:1970CoAsi.239....1B.{{cite journal}}: CS1 maint: multiple names: authors list (link)