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HD 224801

From Wikipedia, the free encyclopedia
Alpha2 Canum Venaticorum variable star in the constellation of Andromeda
HD 224801

Alight curve for CG Andromedae (HD 224801), plotted fromTESS data.[1]
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension00h 00m 43.6345s[2]
Declination+45° 15′ 12.007″[2]
Apparent magnitude (V)6.32 – 6.42[3]
Characteristics
Spectral typeA0IIspSiSrHg[4]
Apparent magnitude (B)6.299[5]
Apparent magnitude (V)6.347[5]
Apparent magnitude (G)6.333[2]
Apparent magnitude (J)6.407[6]
Apparent magnitude (H)6.506[6]
Apparent magnitude (K)6.511[6]
U−Bcolor index-0.35[7]
B−Vcolor index-0.0425[5]
Variable typeAlpha² CVn[8]
Astrometry
Radial velocity (Rv)−1.00±2.2[9] km/s
Proper motion (μ)RA: +17.745[2]mas/yr
Dec.: +0.607[2]mas/yr
Parallax (π)5.5784±0.0405 mas[2]
Distance585 ± 4 ly
(179 ± 1 pc)
Absolute magnitude (MV)0.0[10]
Details
Mass3.4[2] M
Radius2.8[2] R
Luminosity170[2] L
Surface gravity (log g)4.12[2] cgs
Temperature11,900[11] K
Metallicity [Fe/H]0.98[10] dex
Rotation3.74[11] days
Rotational velocity (v sin i)30[7] km/s
Age239[12] Myr
Other designations
CG Andromedae,BD+44° 4538,HD 224801,HIP 63,HR 9080,SAO 53568,PPM 42458,TYC 3246-2388-1.
Database references
SIMBADdata

HD 224801, also known asCG Andromedae, is anAlpha2 Canum Venaticorum variablestar in the constellationAndromeda. Located approximately 188 parsecs (610 ly) away, the star varies betweenapparent magnitudes 6.32 and 6.42 over a period of approximately 3.74 days.

Spectrum

[edit]

CG Andromedae is also a chemically peculiar star with a strong magnetic field, orAp star, with aspectral type A0IIspSiSrHg. This means that it's abright giant star that shows narrowabsorption lines and unusual strong lines ofsilicium,strontium andmercury.Calcium andmanganese lines are weaker than expected instead.[4] Other sources report that the stronger lines are ofsilicium andeuropium, thus giving a spectral classification B9pSiEu, which has just a slightly different temperature for theblackbody emission in addition to the different lines.[3]

Variability

[edit]

CG Andromedae's variability was detected in 1951, and announced by Sanford S. Provin in 1953.[13]

Like inAlpha2 Canum Venaticorum variable stars, CG Andromedae shows a variation of luminosity and one in the strength of spectral lines with the same period of approximately 3.74 days.[8] It is thought that this is caused by an inhomogeneous distribution of elements on the surface of the star, which cause an inhomogeneous surface brightness.

A shorter period, slightly longer than 2 hours, with an amplitude of 0.011 magnitudes has been observed in thelight curve of CG Andromedae; however, with a temperature of 11,000K, it lies outside the instability strip of theHR diagram whererapidly oscillating Ap stars are located.Magnetohydrodynamic waves propagating in the star could explain the observed variability.[4]

References

[edit]
  1. ^"MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved30 October 2024.
  2. ^abcdefghijVallenari, 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 atVizieR.
  3. ^abCG And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al.,CDS IDII/250 Accessed on line 2018-10-17.
  4. ^abcAbt, H. A.; Morrell, N. A. (1995)."The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars".Astrophysical Journal Supplement.99: 135.Bibcode:1995ApJS...99..135A.doi:10.1086/192182.
  5. ^abcHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy & Astrophysics.355:L27 –L30.Bibcode:2000A&A...355L..27H.
  6. ^abcCutri, Roc M.; Skrutskie, Michael F.; Van Dyk, Schuyler D.; Beichman, Charles A.; Carpenter, John M.; Chester, Thomas; Cambresy, Laurent; Evans, Tracey E.; Fowler, John W.; Gizis, John E.; Howard, Elizabeth V.; Huchra, John P.; Jarrett, Thomas H.; Kopan, Eugene L.; Kirkpatrick, J. Davy; Light, Robert M.; Marsh, Kenneth A.; McCallon, Howard L.; Schneider, Stephen E.; Stiening, Rae; Sykes, Matthew J.; Weinberg, Martin D.; Wheaton, William A.; Wheelock, Sherry L.; Zacarias, N. (2003)."VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)".CDS/ADC Collection of Electronic Catalogues.2246: II/246.Bibcode:2003yCat.2246....0C.
  7. ^abRenson, P.; Manfroid, J. (2009)."Catalogue of Ap, HgMn and Am stars".Astronomy and Astrophysics.498 (3):961–966.Bibcode:2009A&A...498..961R.doi:10.1051/0004-6361/200810788.
  8. ^abVSX (4 January 2010)."CG Andromedae".AAVSO Website.American Association of Variable Star Observers. Retrieved9 October 2014.
  9. ^Gontcharov, G. A. (November 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.
  10. ^abAnderson, 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.
  11. ^abShultz, M. E.; Owocki, S. P.; Ud-Doula, A.; Biswas, A.; Bohlender, D.; Chandra, P.; Das, B.; David-Uraz, A.; Khalack, V.; Kochukhov, O.; Landstreet, J. D.; Leto, P.; Monin, D.; Neiner, C.; Rivinius, Th; Wade, G. A. (2022)."MOBSTER - VI. The crucial influence of rotation on the radio magnetospheres of hot stars".Monthly Notices of the Royal Astronomical Society.513 (1): 1429.arXiv:2201.05512.Bibcode:2022MNRAS.513.1429S.doi:10.1093/mnras/stac136.
  12. ^Gontcharov, G. A. (December 2012). "Dependence of kinematics on the age of stars in the solar neighborhood".Astronomy Letters.38 (12):771–782.arXiv:1606.08814.Bibcode:2012AstL...38..771G.doi:10.1134/S1063773712120031.ISSN 0320-0108.S2CID 255201789.
  13. ^Provin, Sanford S. (November 1953)."Light-Variations of Peculiar a Stars".Astrophysical Journal.118: 489.Bibcode:1953ApJ...118..489P.doi:10.1086/145777. Retrieved30 October 2024.
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