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S Pegasi

S Pegasi

The visual band light curve of S Pegasi, from AAVSO data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Pegasus
Right ascension 23h 20m 32.61474s[2]
Declination +08° 55′ 08.1627″[2]
Apparent magnitude (V) 6.9–13.8[3]
Characteristics
Spectral type M5e – M8.5e[3]
Variable type Mira[3]
Astrometry
Radial velocity (Rv)5.0±4.6[4] km/s
Proper motion (μ) RA: −18.494 mas/yr[2]
Dec.: −17.197 mas/yr[2]
Parallax (π)1.399 ± 0.083 mas[5]
Distance2,300 ± 100 ly
(710 ± 40 pc)
Details
Radius278–316[5] R
Luminosity6,545+583
−531
[5] L
Surface gravity (log g)−0.45 to −0.39[5] cgs
Temperature2,910–2,932[5] K
Other designations
S Peg, BD+08° 5047a, HD 220033, HIP 115242
Database references
SIMBADdata

S Pegasi (S Peg) is a Mira variable star in the constellation Pegasus. It varies between magnitude 7 and 13 with a period of 319.22 days.[3] It is believed to be pulsating in the first overtone. First overtone pulsators have masses less than 1.8 M at a temperature of 2,107 K, and less than 1.4 M at the luminosity of S Pegasi.[6]

References

  1. ^ "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
  2. ^ a b c 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. ^ a b c d 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. Bibcode:2009yCat....102025S.
  4. ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 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.
  5. ^ a b c d e Béguin, E.; Chiavassa, A.; Ahmad, A.; Freytag, B.; Uttenthaler, S. (2024-10-01). "Retrieving stellar parameters and dynamics of AGB stars with Gaia parallax measurements and CO5BOLD RHD simulations". Astronomy & Astrophysics. 690: A125. arXiv:2409.03422. doi:10.1051/0004-6361/202450245. ISSN 0004-6361.
  6. ^ Serkowski, Krzysztof; Shawl, Stephen J. (2001). "Polarimetry of 167 Cool Variable Stars: Data". The Astronomical Journal. 122 (4): 2017. Bibcode:2001AJ....122.2017S. doi:10.1086/323105.


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