HD 23277

Last updated
HD 23277
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Camelopardalis [1]
Right ascension 03h 49m 13.7393s [2]
Declination +70° 52′ 15.781″ [2]
Apparent magnitude  (V)5.391 ± 0.009 [3]
Characteristics
Spectral type kA2hA6VmA7 [4]
U−B color index +0.12 [5]
B−V color index +0.09 [5]
Astrometry
Radial velocity (Rv)17 ± 0.9 [6] km/s
Proper motion (μ)RA: 21.451(45) mas/yr [2]
Dec.: −62.431(55) mas/yr [2]
Parallax (π)8.7759±0.0632  mas [2]
Distance 372 ± 3  ly
(113.9 ± 0.8  pc)
Absolute magnitude  (MV)+0.27 [1]
Orbit [7]
PrimaryHD 23277 A
CompanionHD 23277 B
Period (P)15.5132 d
Semi-major axis (a)43.0229 AU
Eccentricity (e)0.2210
Argument of periastron (ω)
(secondary)		287.41°
Argument of periastron (ω)
(primary)		107.41°
Semi-amplitude (K1)
(primary)		22.20 km/s
Semi-amplitude (K2)
(secondary)		24.69 km/s
Details
A
Mass 2.38 ± 0.13 [8]   M☉
Radius 3.55+0.16
−0.24 [8]   R☉
Luminosity 59.7 [9]   L☉
Surface gravity (log g)3.72 ± 0.08 [8]   cgs
Temperature 8,317+194
−189 [8]   K
Rotational velocity (v sin i)25 ± 5 [10]  km/s
Age 610 [11]   Myr
B
Mass 2.11 [7]   M☉
Rotational velocity (v sin i)25 ± 5 [10]  km/s
Other designations
BD+70°257, HD 23277, HIP 17854, HR 1138, SAO 5000
Database references
SIMBAD data

HD 23277 (HR 1138) is a spectroscopic binary [12] located in the northern circumpolar constellation Camelopardalis. With a combined apparent magnitude of 5.39, [3] it is faintly visible to the naked eye under ideal conditions. This star is located at a distance of 372 light years, [2] but is drifting away at a rate of 17 km/s. [6]

The primary has a classification of kA2hA6VmA7, [4] which indicates that it has the calcium K-line of an A2 star, but its hydrogen lines suggest a class of A6 V and metallic lines of an A7 star. At present it has 2.38 times the Sun's mass, and 3.55 times its radius. [8] It radiates at 59.7 times the luminosity of the Sun [9] from its photosphere at an effective temperature of 8,317  K , [8] which gives it a white hue. The companion has 2.11 times the Sun's mass, [7] which suggests it is an A-type main-sequence star like the primary. Both stars spin at a projected rotational velocity of 25 km/s, common for an Am star. [10]

References

  1. 1 2 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters . 38 (5): 331. arXiv: 1108.4971 . Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR.
  2. 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211 . Bibcode:2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940 . S2CID   244398875. Gaia DR3 record for this source at VizieR.
  3. 1 2 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27 –L30. Bibcode:2000A&A...355L..27H. ISSN   0004-6361.
  4. 1 2 Abt, Helmut A.; Morrell, Nidia I. (July 1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". The Astrophysical Journal Supplement Series. 99: 135. Bibcode:1995ApJS...99..135A. doi: 10.1086/192182 . ISSN   0067-0049.
  5. 1 2 Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
  6. 1 2 Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Carnegie Institute Washington D.C. Publication: 0. Bibcode:1953GCRV..C......0W.
  7. 1 2 3 Kraicheva, Z.; Popova, E.; Tutukov, A.; Yungelson, L. (July 1980). "Catalogue of physical parameters of spectroscopic binary stars". Bulletin d'Information du Centre de Donnees Stellaires. 19: 71. Bibcode:1980BICDS..19...71K. ISSN   1169-8837.
  8. 1 2 3 4 5 6 Allende Prieto, C.; Lambert, D. L. (December 1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555–562. arXiv: astro-ph/9911002 . Bibcode:1999A&A...352..555A. ISSN   0004-6361.
  9. 1 2 McDonald, I.; Zijlstra, A. A.; Watson, R. A. (October 2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars". Monthly Notices of the Royal Astronomical Society. 471 (1): 770–791. arXiv: 1706.02208 . Bibcode:2017MNRAS.471..770M. doi: 10.1093/mnras/stx1433 . ISSN   0035-8711.
  10. 1 2 3 Howe, K. S.; Clarke, C. J. (January 2009). "An analysis of v sin (i) correlations in early-type binaries". Monthly Notices of the Royal Astronomical Society. 392 (1): 448–454. Bibcode:2009MNRAS.392..448H. doi: 10.1111/j.1365-2966.2008.14073.x . ISSN   0035-8711.
  11. ↑ "Digital Demo Room - Stellar Structure and Evolution Simulator". rainman.astro.illinois.edu. Retrieved 30 December 2021.
  12. ↑ Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G.; Udry, S. (September 2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics. 424: 727–732. arXiv: astro-ph/0406573 . Bibcode:2004A&A...424..727P. doi: 10.1051/0004-6361:20041213 . ISSN   0004-6361.
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