106 Herculis
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
Right ascension 18h 20m 17.91482s[1]
Declination +21° 57′ 40.6622″[1]
Apparent magnitude (V) 4.96[2]
Characteristics
Spectral type M0 III[3]
U−B color index +1.98[4]
B−V color index +1.58[4]
Variable type suspected SR[5][6]
Astrometry
Radial velocity (Rv)−35.20±0.29[7] km/s
Proper motion (μ) RA: +18.105[1] mas/yr
Dec.: -59.631[1] mas/yr
Parallax (π)8.5067 ± 0.1739 mas[1]
Distance383 ± 8 ly
(118 ± 2 pc)
Absolute magnitude (MV)−0.664[7]
Details
Radius44.32+2.70
−5.89[1] R☉
Luminosity414.1±9.7[1] L☉
Surface gravity (log g)1.56±0.09[3] cgs
Temperature3,789±6[3] K
Metallicity [Fe/H]0.00±0.03[3] dex
Rotational velocity (v sin i)5.0±1.0[8] km/s
Other designations
106 Her, NSV 24405, BD+21°3390, HD 168720, HIP 89861, HR 6868, SAO 85941[9]
Database references
SIMBADdata

106 Herculis is a variable star in the northern constellation Hercules. It is visible to the naked eye as a faint, red-hued point of light with a baseline apparent visual magnitude of 4.96.[2] Based on its parallax, it is estimated to lie 383 light-years (117 parsecs) away from the Sun.[3] The star is moving closer to the Earth with a heliocentric radial velocity of -35 km/s.[7]

Eggleton and Tokovinin (2008) listed this as a suspected binary star system consisting of two roughly equal components.[10] It appears as an ageing red giant with a stellar classification of M0III. This is a suspected semiregular variable star with a very small amplitude and a period of 40 days or more.[6] Having exhausted the supply of hydrogen at its core, it has expanded to 44[1] times the Sun's radius. It is radiating around 414[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of about 3,789 K.[3]

References

  1. ^ a b c d e f g h i 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. Gaia DR2 record for this source at VizieR.
  2. ^ a b J. R., Ducati (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
  3. ^ a b c d e f Wu, Yue; et al. (2010). "Coudé-feed stellar spectral library – atmospheric parameters". Astronomy & Astrophysics. 525: A71. arXiv:1009.1491. Bibcode:2011A&A...525A..71W. doi:10.1051/0004-6361/201015014. S2CID 53480665.
  4. ^ a b Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
  5. ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1: B/gcvs. Bibcode:2009yCat....102025S.
  6. ^ a b Percy, John R. (1993). "The photometric variability of K giants". Publications of the Astronomical Society of the Pacific. 105: 1422. Bibcode:1993PASP..105.1422P. doi:10.1086/133324.
  7. ^ a b c Soubiran, C.; Bienaymé, O.; Mishenina, T. V.; Kovtyukh, V. V. (2008). "Vertical distribution of Galactic disk stars". Astronomy & Astrophysics. 480 (1): 91–101. arXiv:0712.1370. Bibcode:2008A&A...480...91S. doi:10.1051/0004-6361:20078788. S2CID 16602121.
  8. ^ Zamanov, R. K.; et al. (October 2008). "Rotational velocities of the giants in symbiotic stars - III. Evidence of fast rotation in S-type symbiotics". Monthly Notices of the Royal Astronomical Society. 390 (1): 377–382. arXiv:0807.3817. Bibcode:2008MNRAS.390..377Z. doi:10.1111/j.1365-2966.2008.13751.x. S2CID 118697261.
  9. ^ "106 Her". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-06-17.
  10. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
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