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R Horologii

Location of R Horologii (R) in Horologium
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Horologium
Right ascension 02h 53m 52.77010s [1]
Declination −49° 53′ 22.7305″ [1]
Apparent magnitude (V) 4.7 – 14.3 [2]
Characteristics
Spectral type M5-7e [3]
B−V color index 1.044±0.011 [4]
Variable type Mira [5]
Astrometry
Radial velocity (Rv)+60.0±4.4 [6] km/s
Proper motion (μ) RA: +128.567  mas/ yr [1]
Dec.: +35.766  mas/ yr [1]
Parallax (π)4.3236 ± 0.1524  mas [1]
Distance755.7+31.6
−6.0  ly
(231.8+9.7
−9.3  pc) [7]
Details
Mass0.94 [8]  M☉
Radius635 [9] [a]  R☉
Luminosity8,500 [9]  L☉
Surface gravity (log g)−0.434 [8]  cgs
Temperature2,200 [10] [9]  K
Metallicity [Fe/H]+0.545 [8]  dex
Other designations
R Hor, CD−50° 860, HD 18242, HIP 13502, HR 868 [11]
Database references
SIMBAD data
The light curve of R Horologii from AAVSO V band data [12]

R Horologii is a red giant star approximately 760 light-years away in the southern constellation of Horologium. [13] It is a Mira variable with a period of 404.83 days, [14] ranging from apparent magnitude 4.7 to 14.3—one of the largest ranges in brightness known of stars in the night sky visible to the unaided eye. [2] The star is losing mass at the rate of 5.9×10−7 M☉·y−1. [10]

Notes

  1. ^ Applying the Stefan–Boltzmann law with a nominal solar effective temperature of 5,772  K:
    .

References

  1. ^ a b c d 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.
  2. ^ a b Privett, Grant; Jones, Kevin (2013). The Constellation Observing Atlas. New York, New York: Springer Science & Business Media. p. 102. ISBN  9781461476481.
  3. ^ Keenan, Philip C. (June 1966). "A Catalogue of Spectra of Mira Variables of Types ME and Se". Astrophysical Journal Supplement. 13: 333. Bibcode: 1966ApJS...13..333K. doi: 10.1086/190139.
  4. ^ 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, S2CID  119257644.
  5. ^ 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. S2CID  125853869.
  6. ^ Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system", Astronomy Letters, 32 (11): 759–771, arXiv: 1606.08053, Bibcode: 2006AstL...32..759G, doi: 10.1134/S1063773706110065, S2CID  119231169.
  7. ^ Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (2021-03-01). "Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3". The Astronomical Journal. 161 (3): 147. arXiv: 2012.05220. Bibcode: 2021AJ....161..147B. doi: 10.3847/1538-3881/abd806. ISSN  0004-6256. Data about this star can be seen here.
  8. ^ a b c Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; de Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv: 1904.11302. Bibcode: 2019A&A...628A..94A. doi: 10.1051/0004-6361/201935765. ISSN  0004-6361.
  9. ^ a b c Danilovich, T.; Teyssier, D.; Justtanont, K.; Olofsson, H.; Cerrigone, L.; Bujarrabal, V.; Alcolea, J.; Cernicharo, J.; Castro-Carrizo, A.; García-Lario, P.; Marston, A. (2015-09-01). "New observations and models of circumstellar CO line emission of AGB stars in the Herschel SUCCESS programme". Astronomy & Astrophysics. 581: A60. arXiv: 1506.09065. doi: 10.1051/0004-6361/201526705. ISSN  0004-6361.
  10. ^ a b Danilovich, T.; et al. (October 2017), "Sulphur-bearing molecules in AGB stars. I. The occurrence of hydrogen sulphide", Astronomy & Astrophysics, 606: 14, arXiv: 1707.06003, Bibcode: 2017A&A...606A.124D, doi: 10.1051/0004-6361/201731203, S2CID  55533463, A124
  11. ^ "R Horologii". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 18 March 2016.
  12. ^ "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
  13. ^ van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv: 0708.1752. Bibcode: 2007A&A...474..653V. doi: 10.1051/0004-6361:20078357. S2CID  18759600.
  14. ^ Templeton, M. R.; Mattei, J. A.; Willson, L. A. (2005). "Secular Evolution in Mira Variable Pulsations". The Astronomical Journal. 130 (2): 776–788. arXiv: astro-ph/0504527. Bibcode: 2005AJ....130..776T. doi: 10.1086/431740. S2CID  359940.
Stub icon

This variable star–related article is a stub. You can help Wikipedia by expanding it.

Retrieved from " https://en.wikipedia.org/?title=R_Horologii&oldid=1234580189"
From Wikipedia, the free encyclopedia
R Horologii

Location of R Horologii (R) in Horologium
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Horologium
Right ascension 02h 53m 52.77010s [1]
Declination −49° 53′ 22.7305″ [1]
Apparent magnitude (V) 4.7 – 14.3 [2]
Characteristics
Spectral type M5-7e [3]
B−V color index 1.044±0.011 [4]
Variable type Mira [5]
Astrometry
Radial velocity (Rv)+60.0±4.4 [6] km/s
Proper motion (μ) RA: +128.567  mas/ yr [1]
Dec.: +35.766  mas/ yr [1]
Parallax (π)4.3236 ± 0.1524  mas [1]
Distance755.7+31.6
−6.0  ly
(231.8+9.7
−9.3  pc) [7]
Details
Mass0.94 [8]  M☉
Radius635 [9] [a]  R☉
Luminosity8,500 [9]  L☉
Surface gravity (log g)−0.434 [8]  cgs
Temperature2,200 [10] [9]  K
Metallicity [Fe/H]+0.545 [8]  dex
Other designations
R Hor, CD−50° 860, HD 18242, HIP 13502, HR 868 [11]
Database references
SIMBAD data
The light curve of R Horologii from AAVSO V band data [12]

R Horologii is a red giant star approximately 760 light-years away in the southern constellation of Horologium. [13] It is a Mira variable with a period of 404.83 days, [14] ranging from apparent magnitude 4.7 to 14.3—one of the largest ranges in brightness known of stars in the night sky visible to the unaided eye. [2] The star is losing mass at the rate of 5.9×10−7 M☉·y−1. [10]

Notes

  1. ^ Applying the Stefan–Boltzmann law with a nominal solar effective temperature of 5,772  K:
    .

References

  1. ^ a b c d 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.
  2. ^ a b Privett, Grant; Jones, Kevin (2013). The Constellation Observing Atlas. New York, New York: Springer Science & Business Media. p. 102. ISBN  9781461476481.
  3. ^ Keenan, Philip C. (June 1966). "A Catalogue of Spectra of Mira Variables of Types ME and Se". Astrophysical Journal Supplement. 13: 333. Bibcode: 1966ApJS...13..333K. doi: 10.1086/190139.
  4. ^ 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, S2CID  119257644.
  5. ^ 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. S2CID  125853869.
  6. ^ Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system", Astronomy Letters, 32 (11): 759–771, arXiv: 1606.08053, Bibcode: 2006AstL...32..759G, doi: 10.1134/S1063773706110065, S2CID  119231169.
  7. ^ Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (2021-03-01). "Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3". The Astronomical Journal. 161 (3): 147. arXiv: 2012.05220. Bibcode: 2021AJ....161..147B. doi: 10.3847/1538-3881/abd806. ISSN  0004-6256. Data about this star can be seen here.
  8. ^ a b c Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; de Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv: 1904.11302. Bibcode: 2019A&A...628A..94A. doi: 10.1051/0004-6361/201935765. ISSN  0004-6361.
  9. ^ a b c Danilovich, T.; Teyssier, D.; Justtanont, K.; Olofsson, H.; Cerrigone, L.; Bujarrabal, V.; Alcolea, J.; Cernicharo, J.; Castro-Carrizo, A.; García-Lario, P.; Marston, A. (2015-09-01). "New observations and models of circumstellar CO line emission of AGB stars in the Herschel SUCCESS programme". Astronomy & Astrophysics. 581: A60. arXiv: 1506.09065. doi: 10.1051/0004-6361/201526705. ISSN  0004-6361.
  10. ^ a b Danilovich, T.; et al. (October 2017), "Sulphur-bearing molecules in AGB stars. I. The occurrence of hydrogen sulphide", Astronomy & Astrophysics, 606: 14, arXiv: 1707.06003, Bibcode: 2017A&A...606A.124D, doi: 10.1051/0004-6361/201731203, S2CID  55533463, A124
  11. ^ "R Horologii". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 18 March 2016.
  12. ^ "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
  13. ^ van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv: 0708.1752. Bibcode: 2007A&A...474..653V. doi: 10.1051/0004-6361:20078357. S2CID  18759600.
  14. ^ Templeton, M. R.; Mattei, J. A.; Willson, L. A. (2005). "Secular Evolution in Mira Variable Pulsations". The Astronomical Journal. 130 (2): 776–788. arXiv: astro-ph/0504527. Bibcode: 2005AJ....130..776T. doi: 10.1086/431740. S2CID  359940.
Stub icon

This variable star–related article is a stub. You can help Wikipedia by expanding it.

Retrieved from " https://en.wikipedia.org/?title=R_Horologii&oldid=1234580189"

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