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YZ Cassiopeiae

Coordinates:Sky map00h 45m 39.0777s, +74° 59′ 17.063″
From Wikipedia, the free encyclopedia
Triple star system in the constellation Cassiopeia
YZ Cas
Location of YZ Cassiopeiae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationCassiopeia[1]
A
Right ascension00h 45m 39.0777s[2]
Declination+74° 59′ 17.063″[2]
Apparent magnitude (V)5.653[3]
B
Right ascension00h 45m 42,1503s[4]
Declination+74° 58′ 43.242″[4]
Apparent magnitude (V)11.23[5]
Characteristics
A
Spectral typeA2IV[6] (A1Vm + F2V[7])
U−Bcolor index+0.07[5]
B−Vcolor index+0.05[5]
Variable typeAlgol[8]
B
Spectral typeF2V[9]
U−Bcolor index+0.64[5]
B−Vcolor index+0.94[5]
Astrometry
Radial velocity (Rv)+8.90±0.4[10] km/s
Proper motion (μ)RA: −15.07[2]mas/yr
Dec.: −22.17[2]mas/yr
Parallax (π)11.24±0.55 mas[2]
Distance103.8[9] pc
Absolute magnitude (MV)+0.251[7]
Orbit[11]
CompanionTYC 4307-2168-1
Period (P)86 580 yr
Orbit[9]
PrimaryAa
CompanionAb
Period (P)4.467 days
Semi-major axis (a)17.47 R[12]
Eccentricity (e)0.0
Inclination (i)88.332°
Details
Aa
Mass2.308[12] M
Radius2.547[12] R
Luminosity41.69[12] L
Surface gravity (log g)3.988[9] cgs
Temperature9,200[12] K
Rotational velocity (v sin i)29.2[9] km/s
Ab
Mass1.325[13] M
Radius1.359[12] R
Luminosity3.34[12] L
Surface gravity (log g)4.311[9] cgs
Temperature6,890[13] K
Metallicity[Fe/H]+0.10[13] dex
Rotational velocity (v sin i)15.0[9] km/s
Age490 - 550[9] Myr
Other designations
21 Cassiopeiae,HR 192,BD+74 27,HD 4161,SAO 4216,HIP 3572,GC 891,ADS 624 A,CCDM J00457+7459[14]
Database references
SIMBADdata

YZ Cassiopeiae (21 Cas) is astar system 103.8parsecs (339 ly) away fromEarth, in the constellationCassiopeia. It comprises three stars: an eclipsingAlgol-type binary and a visually fainter star about 3000AU distant.[11] It is faintly visible to thenaked eye under good observing conditions.

Alight curve for YZ Cassiopeiae, plotted fromTESS data[15]

The primary star in the YZ Cassiopeiae system is a whitesubgiant (main sequence) star ofspectral type A1Vm and 2.31 solar masses[11] (M) with a less massive main sequence dwarf star of type F2V[3] and 1.35M.[11]

In 1924, Joel Stebbins announced his discovery that the star, then known as 21 Cassiopeiae, is aneclipsing binary.[16] It was given itsvariable star designation, YZ Cassiopeiae, in 1925.[17] Theapparent magnitude of the eclipsing binary varies from 5.65 to 6.05[3] with a period of 4.4672 days.[11] Combined, they appear to have a spectral type of A2IV.[11]

The binary has a dimmer (magnitude 9.7 according to Norton,[18] or 10.5 by SIMBAD) companion of 0.8M[11] orbiting with a period of about 86 580 years.[11]

References

[edit]
  1. ^Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5):331–346.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.eISSN 1562-6873.ISSN 1063-7737.S2CID 119257644.
  2. ^abcdevan 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. ^abcJerzy M. Kreiner, Chun-Hwey Kim, Il-Seong Nha.YZ CAS: Atlas of O-C Diagrams of Eclipsing Binary Stars
  4. ^abHog, E.; Kuzmin, A.; Bastian, U.; Fabricius, C.; Kuimov, K.; Lindegren, L.; Makarov, V. V.; Roeser, S. (1998). "The TYCHO Reference Catalogue".Astronomy and Astrophysics.335: L65.Bibcode:1998A&A...335L..65H.
  5. ^abcdeEggen, O. J. (1963). "Three-color photometry of the components in 228 wide double and multiple systems".Astronomical Journal.68: 483.Bibcode:1963AJ.....68..483E.doi:10.1086/109000.
  6. ^Grenier, S.; Baylac, M.-O.; Rolland, L.; Burnage, R.; Arenou, F.; Briot, D.; Delmas, F.; Duflot, M.; Genty, V.; Gómez, A. E.; Halbwachs, J.-L.; Marouard, M.; Oblak, E.; Sellier, A. (1999)."Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS"(PDF).Astronomy and Astrophysics Supplement.137 (3): 451.Bibcode:1999A&AS..137..451G.doi:10.1051/aas:1999489.
  7. ^abBilir, S.; Ak, T.; Soydugan, E.; Soydugan, F.; Yaz, E.; Filiz Ak, N.; Eker, Z.; Demircan, O.; Helvaci, M. (2008). "New absolute magnitude calibrations for detached binaries".Astronomische Nachrichten.329 (8): 835.arXiv:0806.1290.Bibcode:2008AN....329..835B.doi:10.1002/asna.200811002.S2CID 6131326.
  8. ^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.
  9. ^abcdefghPavlovski, K.; Southworth, J.; Kolbas, V.; Smalley, B. (2014)."Absolute dimensions of detached eclipsing binaries - III. The metallic-lined system YZ Cassiopeiae".Monthly Notices of the Royal Astronomical Society.438 (1):590–603.arXiv:1311.3482.Bibcode:2014MNRAS.438..590P.doi:10.1093/mnras/stt2229.S2CID 56144135.
  10. ^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.
  11. ^abcdefghTokovinin 1997-1999.J/A+AS/124/75. Multiple star catalogue (MSC)
  12. ^abcdefgEker, Z.; Soydugan, F.; Soydugan, E.; Bilir, S.; Yaz Gökçe, E.; Steer, I.; Tüysüz, M.; Şenyüz, T.; Demircan, O. (2015). "Main-Sequence Effective Temperatures from a Revised Mass-Luminosity Relation Based on Accurate Properties".The Astronomical Journal.149 (4): 131.arXiv:1501.06585.Bibcode:2015AJ....149..131E.doi:10.1088/0004-6256/149/4/131.S2CID 118740259.
  13. ^abcMaxted, P. F. L.; Serenelli, A. M.; Southworth, J. (2015). "Bayesian mass and age estimates for transiting exoplanet host stars".Astronomy & Astrophysics.575: A36.arXiv:1412.7891.Bibcode:2015A&A...575A..36M.doi:10.1051/0004-6361/201425331.S2CID 54857801.
  14. ^"V* YZ Cas".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved26 January 2018.
  15. ^"MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved8 December 2021.
  16. ^Stebbins, Joel (1924)."Photo-electric photometry at the Washburn Observatory".Popular Astronomy.32:233–234.Bibcode:1924PA.....32..233S. Retrieved14 January 2025.
  17. ^Guthnick, P.; Prager, R. (March 1925)."Benennung von neu entdeckten veränderlichen Sternen".Astronomische Nachrichten.224 (8):129–148.Bibcode:1925AN....224..129G.doi:10.1002/asna.19252240802. Retrieved14 January 2025.
  18. ^Norton, Arthur P. (1973).Norton's Star Atlas. Gall & Inglis. p. 118.ISBN 0-85248-900-5.


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