HD 153261

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HD 153261
HD153261LightCurve.png
A light curve for HD 153261 from Hipparcos data, adapted from Lefèvre et al. (2009) [1]
Observation data
Epoch J2000       Equinox J2000
Constellation Ara
Right ascension 17h 01m 47.3875s [2]
Declination –58° 57′ 29.681″ [2]
Apparent magnitude  (V)6.137 [3]
Characteristics
Spectral type B1 V:ne [4] or B2 IVne [5]
U−B color index –0.956 [3]
B−V color index –0.078 [3]
Astrometry
Radial velocity (Rv)–6 [6] km/s
Proper motion (μ)RA: –2.91 [2] mas/yr
Dec.: –9.01 [2] mas/yr
Parallax (π)2.32±0.38  mas [2]
Distance approx. 1,400  ly
(approx. 430  pc)
Details
Mass 10.1 ± 0.3 [5]   M☉
Radius 4.5 [7]   R☉
Luminosity (bolometric)11,045 [8]   L☉
Temperature 21,150 [8]   K
Age 20.4 ± 0.4 [5]   Myr
Other designations
CD–58 6607, HD 153261, HIP 83323, HR  6304, SAO 244362, V828 Arae. [9]
Database references
SIMBAD data

HD 153261 is the Henry Draper Catalogue designation for a star in the southern constellation of Ara. It has an apparent visual magnitude of 6.137, [3] placing it near the threshold of naked eye visibility. According to the Bortle Dark-Sky Scale, it can be viewed from dark suburban or rural skies. Based upon an annual parallax shift of just 2.32  mas, [2] it is located at a distance of around 1,400 light-years (430 parsecs ) from Earth.

In 1983, Christopher Stagg reported that he suspected that HD 153261 is a variable star, and his later observations confirmed that it is in fact variable. [10] [11] HD 153261 was given its variable star designation, V828 Arae, in 1987. [12]

This star has been catalogued with a stellar classification of B1 V:ne [4] or B2 IVne, [5] indicating that it is either a main sequence or a subgiant star. The 'n' indicates a nebulous spectrum created by the Doppler shift-broadened absorption lines from a rapid rotation, while the 'e' means this is a Be star, with the spectrum showing emission lines from hot, circumstellar gas. HD 153261 displays some variability with an amplitude of 0.090 in magnitude, and is a suspected spectroscopic binary. [1]

HD 153261 is a large star with over ten [5] times the Sun's mass and around 4.5 [7] the radius of the Sun. It shines with more than 11,000 [8] times the brightness of the Sun, with this energy being radiated into space at an effective temperature of 21,150 K. [8] At this heat, it glows with the blue-white hue of a B-type star. [13]

References

  1. 1 2 Lefèvre, L.; et al. (November 2009), "A systematic study of variability among OB-stars based on HIPPARCOS photometry", Astronomy and Astrophysics, 507 (2): 11411201, Bibcode:2009A&A...507.1141L, doi: 10.1051/0004-6361/200912304 .
  2. 1 2 3 4 5 6 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv: 0708.1752 , Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID   18759600.
  3. 1 2 3 4 Kozok, J. R. (September 1985), "Photometric observations of emission B-stars in the southern Milky Way", Astronomy and Astrophysics Supplement Series, 61: 387–405, Bibcode:1985A&AS...61..387K.
  4. 1 2 Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1975mcts.book.....H.
  5. 1 2 3 4 5 Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society , 410 (1): 190–200, arXiv: 1007.4883 , Bibcode:2011MNRAS.410..190T, doi: 10.1111/j.1365-2966.2010.17434.x , S2CID   118629873.
  6. ↑ Evans, D. S. (June 20–24, 1966), "The Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.), Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, vol. 30, University of Toronto: International Astronomical Union, p. 57, Bibcode:1967IAUS...30...57E.
  7. 1 2 Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics, 367 (2): 521–524, arXiv: astro-ph/0012289 , Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID   425754.
  8. 1 2 3 4 Hohle, M. M.; Neuhäuser, R.; Schutz, B. F. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten, 331 (4): 349, arXiv: 1003.2335 , Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID   111387483.
  9. ↑ "HR 6304". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2010-08-03.{{cite web}}: CS1 maint: postscript (link)
  10. ↑ Stagg, C. (1983). "The southern Be star photometric campaign - A first report". Hvar Observatory Bulletin. 7 (1): 143. Bibcode:1983HvaOB...7..143S . Retrieved 25 November 2024.
  11. ↑ Stagg, Christopher (July 1987). "A photometric survey of the bright southern Be stars". Monthly Notices of the Royal Astronomical Society. 227: 213–240. Bibcode:1987MNRAS.227..213S. doi: 10.1093/mnras/227.1.213 . Retrieved 25 November 2024.
  12. ↑ Kholopov, P. N.; Samus, N. N.; Kazarovets, E. V.; Kireeva, N. N. (August 1987). "The 68th Name-List of Variable Stars". Information Bulletin on Variable Stars. 3058: 1. Bibcode:1987IBVS.3058....1K . Retrieved 25 November 2024.
  13. ↑ "The Colour of Stars", Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the original on March 18, 2012, retrieved 2012-07-21.
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