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TY Coronae Borealis

TY Coronae Borealis, also known as Ross 808, is a variable white dwarf star of the DAV (or ZZ Ceti) type in the constellation Corona Borealis. It has a surface temperature of 11,213 ± 130 K and a mass around 70% times that of the Sun, but only 1.1% of its diameter.[5] It is 107 light-years distant from Earth.[2] It was confirmed as a variable star in 1976.[6]

TY Coronae Borealis

A blue band light curve for TY Coronae Borealis, adapted from Bognár et al. (2019)[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Corona Borealis
Right ascension 16h 01m 23.187s[2]
Declination +36° 48′ 34.29″[2]
Apparent magnitude (V) 14.53[3]
Characteristics
Evolutionary stage White dwarf
Spectral type DA4.4[4]
Astrometry
Proper motion (μ) RA: 101.113[2] mas/yr
Dec.: −545.353[2] mas/yr
Parallax (π)30.4668 ± 0.0187 mas[2]
Distance107.05 ± 0.07 ly
(32.82 ± 0.02 pc)
Other designations
TY CrB, Ross 808, WD 1600+369, LTT 14769, NLTT 41782, 2MASS J16012317+3648351[4]
Database references
SIMBADdata

References edit

  1. ^ Bognár, Zs.; Paparó, M.; Sódor, Á.; Jenei, D. I.; Kalup, Cs.; Bertone, E.; Chavez-Dagostino, M.; Montgomery, M. H.; Gyõrffy, Á.; Molnár, L.; Ollé, H.; Pápics, P. I.; Plachy, E.; Verebélyi, E. (January 2019). "Wandering near the red edge: photometric observations of three cool ZZ Ceti stars". Monthly Notices of the Royal Astronomical Society. 482 (3): 4018–4031. arXiv:1810.09711. Bibcode:2019MNRAS.482.4018B. doi:10.1093/mnras/sty2884.
  2. ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  3. ^ Watson, Christopher (4 January 2010). "TY Coronae Borealis". AAVSO Website. American Association of Variable Star Observers. Retrieved 23 November 2014.
  4. ^ a b "TY CrB". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 5 December 2016.
  5. ^ Romero, A. D.; Córsico, A. H.; Althaus, L. G.; Kepler, S. O.; Castanheira, B. G.; Miller Bertolami, M. M. (2012). "Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models". Monthly Notices of the Royal Astronomical Society. 420 (2): 1462–80. arXiv:1109.6682. Bibcode:2012MNRAS.420.1462R. doi:10.1111/j.1365-2966.2011.20134.x. S2CID 55018129.
  6. ^ McGraw, John T.; Robinson, Edward L. (1976). "High-speed photometry of luminosity-variable DA dwarfs: R808, GD 99, and G 117-B15A". Astrophysical Journal Letters. 205: L155-58. Bibcode:1976ApJ...205L.155M. doi:10.1086/182112.


coronae, borealis, also, known, ross, variable, white, dwarf, star, ceti, type, constellation, corona, borealis, surface, temperature, mass, around, times, that, only, diameter, light, years, distant, from, earth, confirmed, variable, star, 1976, blue, band, l. TY Coronae Borealis also known as Ross 808 is a variable white dwarf star of the DAV or ZZ Ceti type in the constellation Corona Borealis It has a surface temperature of 11 213 130 K and a mass around 70 times that of the Sun but only 1 1 of its diameter 5 It is 107 light years distant from Earth 2 It was confirmed as a variable star in 1976 6 TY Coronae BorealisA blue band light curve for TY Coronae Borealis adapted from Bognar et al 2019 1 Observation dataEpoch J2000 0 Equinox J2000 0 Constellation Corona Borealis Right ascension 16h 01m 23 187s 2 Declination 36 48 34 29 2 Apparent magnitude V 14 53 3 Characteristics Evolutionary stage White dwarf Spectral type DA4 4 4 AstrometryProper motion m RA 101 113 2 mas yr Dec 545 353 2 mas yrParallax p 30 4668 0 0187 mas 2 Distance107 05 0 07 ly 32 82 0 02 pc Other designationsTY CrB Ross 808 WD 1600 369 LTT 14769 NLTT 41782 2MASS J16012317 3648351 4 Database referencesSIMBADdataReferences edit Bognar Zs Paparo M Sodor A Jenei D I Kalup Cs Bertone E Chavez Dagostino M Montgomery M H Gyorffy A Molnar L Olle H Papics P I Plachy E Verebelyi E January 2019 Wandering near the red edge photometric observations of three cool ZZ Ceti stars Monthly Notices of the Royal Astronomical Society 482 3 4018 4031 arXiv 1810 09711 Bibcode 2019MNRAS 482 4018B doi 10 1093 mnras sty2884 a b c d e f Brown A G A et al Gaia collaboration 2021 Gaia Early Data Release 3 Summary of the contents and survey properties Astronomy amp Astrophysics 649 A1 arXiv 2012 01533 Bibcode 2021A amp A 649A 1G doi 10 1051 0004 6361 202039657 S2CID 227254300 Erratum doi 10 1051 0004 6361 202039657e Gaia EDR3 record for this source at VizieR Watson Christopher 4 January 2010 TY Coronae Borealis AAVSO Website American Association of Variable Star Observers Retrieved 23 November 2014 a b TY CrB SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 5 December 2016 Romero A D Corsico A H Althaus L G Kepler S O Castanheira B G Miller Bertolami M M 2012 Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models Monthly Notices of the Royal Astronomical Society 420 2 1462 80 arXiv 1109 6682 Bibcode 2012MNRAS 420 1462R doi 10 1111 j 1365 2966 2011 20134 x S2CID 55018129 McGraw John T Robinson Edward L 1976 High speed photometry of luminosity variable DA dwarfs R808 GD 99 and G 117 B15A Astrophysical Journal Letters 205 L155 58 Bibcode 1976ApJ 205L 155M doi 10 1086 182112 nbsp This variable star related article is a stub You can help Wikipedia by expanding it vte nbsp This article about a white dwarf is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title TY Coronae Borealis amp oldid 1134882282, wikipedia, wiki, book, books, library,

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