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HL Tau 76

HL Tau 76 is a variable white dwarf star of the DAV (or ZZ Ceti) type. It was observed by G. Haro and W. J. Luyten in 1961,[8][9] and was the first variable white dwarf discovered when, in 1968, Arlo U. Landolt found that it varied in brightness with a period of approximately 749.5 seconds, or 12.5 minutes.[9] Like other DAV white dwarfs, its variability arises from non-radial gravity wave pulsations within itself.[10], § 7. Later observation and analysis has found HL Tau 76 to pulsate in over 40 independent vibrational modes, with periods between 380 seconds and 1390 seconds.[11]

HL Tau 76

A white-light light curve light curve for HL Tau 76, adapted from Warner and Nather (1972)[1]
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Taurus
Right ascension 04h 18m 56.638s[2]
Declination +27° 17′ 48.31″[2]
Apparent magnitude (V) 14.1–15.28[3]
Characteristics
Spectral type DA4.3[4]
B−V color index 0.2[5]
Variable type DAV (ZZ Ceti)[3]
Astrometry
Proper motion (μ) RA: 62.600[2] mas/yr
Dec.: −72.819[2] mas/yr
Parallax (π)20.7244 ± 0.0338 mas[2]
Distance157.4 ± 0.3 ly
(48.25 ± 0.08 pc)
Absolute magnitude (MV)11.69[4]
Details
Mass0.575±0.005[6] M
Radius0.0162[6] R
Luminosity0.00389[6] L
Surface gravity (log g)7.8[7] cgs
Temperature11,375±30[6] K
Other designations
EGGR 265, V411 Tau, WD 0416+272[5]
Database references
SIMBADdata

The designation HL Tau 76 derives from the discovery of this star as a white dwarf, when it was described as Taurus no.76 in a publication authored by Guillermo Haro and Willem Jacob Luyten.[8] The exact designation HL Tau 76 was then used in subsequent papers, including one giving the star its designation EGGR 265 where it was noted to be variable.[12] It was then included in the 57th name-list of variable stars and given the variable star designation V441 Tauri.[13] The unusual designation HL Tau 76 continues to be used by most authors.[14]

Notes and references edit

  1. ^ Warner, Brian; Nather, R. Edward (January 1972). "Observations of rapid blue variables-III. HL Tau-76". Monthly Notices of the Royal Astronomical Society. 156: 1–5. Bibcode:1972MNRAS.156....1W. doi:10.1093/mnras/156.1.1.
  2. ^ a b c d e 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. ^ a b Combined General Catalogue of Variable Stars (GCVS), v. 4.2. CDS ID II/250.
  4. ^ a b Gianninas, A.; Bergeron, P.; Ruiz, M. T. (2011). "A Spectroscopic Survey and Analysis of Bright, Hydrogen-rich White Dwarfs". The Astrophysical Journal. 743 (2): 138. arXiv:1109.3171. Bibcode:2011ApJ...743..138G. doi:10.1088/0004-637X/743/2/138. S2CID 119210906.
  5. ^ a b "HL Tau 76". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved June 12, 2007.
  6. ^ a b c d Pech, D.; Vauclair, G.; Dolez, N. (2006). "Asteroseismological constraints on the structure of the ZZ Ceti star HL Tau 76". Astronomy and Astrophysics. 446 (1): 223. Bibcode:2006A&A...446..223P. doi:10.1051/0004-6361:20053150.
  7. ^ Gentile Fusillo, N. P.; Tremblay, P. -E.; Cukanovaite, E.; Vorontseva, A.; Lallement, R.; Hollands, M.; Gänsicke, B. T.; Burdge, K. B.; McCleery, J.; Jordan, S. (2021). "A catalogue of white dwarfs in Gaia EDR3". Monthly Notices of the Royal Astronomical Society. 508 (3): 3877. arXiv:2106.07669. Bibcode:2021MNRAS.508.3877G. doi:10.1093/mnras/stab2672.
  8. ^ a b Haro, G.; Luyten, W. J. (1961). "Nueva estrella enana blanca en las nubes obscuras del Toro". Boletín de los Observatorios de Tonantzintla y Tacubaya. 3: 35. Bibcode:1961BOTT....3...35H.
  9. ^ a b Landolt, Arlo U. (1968). "A New Short-Period Blue Variable". The Astrophysical Journal. 153: 151. Bibcode:1968ApJ...153..151L. doi:10.1086/149645.
  10. ^ Koester, D.; Chanmugam, G. (1990). "Physics of white dwarf stars". Reports on Progress in Physics. 53 (7): 837. Bibcode:1990RPPh...53..837K. doi:10.1088/0034-4885/53/7/001. S2CID 250915046.
  11. ^ Dolez, N.; et al. (2006). "Whole Earth telescope observations of the ZZ Ceti star HL Tau 76". Astronomy and Astrophysics. 446 (1): 237. Bibcode:2006A&A...446..237D. doi:10.1051/0004-6361:20053149.
  12. ^ Greenstein, Jesse L. (October 1969). "The Lowell Suspect White Dwarfs". Astrophysical Journal. 158: 281. Bibcode:1969ApJ...158..281G. doi:10.1086/150191.
  13. ^ Kukarkin, B. V.; et al. (October 1970). "57th Name-List of Variable Stars". Information Bulletin on Variable Stars. 480 (1): 1. Bibcode:1970IBVS..480....1K.
  14. ^ Chen, Y. H.; Shu, H. (January 2021). "Asteroseismology of the DAV star R808". Monthly Notices of the Royal Astronomical Society. 500 (4): 4703–4709. arXiv:2011.06918. Bibcode:2021MNRAS.500.4703C. doi:10.1093/mnras/staa3572.

confused, with, tauri, variable, white, dwarf, star, ceti, type, observed, haro, luyten, 1961, first, variable, white, dwarf, discovered, when, 1968, arlo, landolt, found, that, varied, brightness, with, period, approximately, seconds, minutes, like, other, wh. Not to be confused with HL Tauri HL Tau 76 is a variable white dwarf star of the DAV or ZZ Ceti type It was observed by G Haro and W J Luyten in 1961 8 9 and was the first variable white dwarf discovered when in 1968 Arlo U Landolt found that it varied in brightness with a period of approximately 749 5 seconds or 12 5 minutes 9 Like other DAV white dwarfs its variability arises from non radial gravity wave pulsations within itself 10 7 Later observation and analysis has found HL Tau 76 to pulsate in over 40 independent vibrational modes with periods between 380 seconds and 1390 seconds 11 HL Tau 76A white light light curve light curve for HL Tau 76 adapted from Warner and Nather 1972 1 Observation dataEpoch J2000 0 Equinox J2000 0 ICRS Constellation TaurusRight ascension 04h 18m 56 638s 2 Declination 27 17 48 31 2 Apparent magnitude V 14 1 15 28 3 CharacteristicsSpectral type DA4 3 4 B V color index 0 2 5 Variable type DAV ZZ Ceti 3 AstrometryProper motion m RA 62 600 2 mas yr Dec 72 819 2 mas yrParallax p 20 7244 0 0338 mas 2 Distance157 4 0 3 ly 48 25 0 08 pc Absolute magnitude MV 11 69 4 DetailsMass0 575 0 005 6 M Radius0 0162 6 R Luminosity0 00389 6 L Surface gravity log g 7 8 7 cgsTemperature11 375 30 6 KOther designationsEGGR 265 V411 Tau WD 0416 272 5 Database referencesSIMBADdataThe designation HL Tau 76 derives from the discovery of this star as a white dwarf when it was described as Taurus no 76 in a publication authored by Guillermo Haro and Willem Jacob Luyten 8 The exact designation HL Tau 76 was then used in subsequent papers including one giving the star its designation EGGR 265 where it was noted to be variable 12 It was then included in the 57th name list of variable stars and given the variable star designation V441 Tauri 13 The unusual designation HL Tau 76 continues to be used by most authors 14 Notes and references edit Warner Brian Nather R Edward January 1972 Observations of rapid blue variables III HL Tau 76 Monthly Notices of the Royal Astronomical Society 156 1 5 Bibcode 1972MNRAS 156 1W doi 10 1093 mnras 156 1 1 a b c d e 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 a b Combined General Catalogue of Variable Stars GCVS v 4 2 CDS ID II 250 a b Gianninas A Bergeron P Ruiz M T 2011 A Spectroscopic Survey and Analysis of Bright Hydrogen rich White Dwarfs The Astrophysical Journal 743 2 138 arXiv 1109 3171 Bibcode 2011ApJ 743 138G doi 10 1088 0004 637X 743 2 138 S2CID 119210906 a b HL Tau 76 SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved June 12 2007 a b c d Pech D Vauclair G Dolez N 2006 Asteroseismological constraints on the structure of the ZZ Ceti star HL Tau 76 Astronomy and Astrophysics 446 1 223 Bibcode 2006A amp A 446 223P doi 10 1051 0004 6361 20053150 Gentile Fusillo N P Tremblay P E Cukanovaite E Vorontseva A Lallement R Hollands M Gansicke B T Burdge K B McCleery J Jordan S 2021 A catalogue of white dwarfs in Gaia EDR3 Monthly Notices of the Royal Astronomical Society 508 3 3877 arXiv 2106 07669 Bibcode 2021MNRAS 508 3877G doi 10 1093 mnras stab2672 a b Haro G Luyten W J 1961 Nueva estrella enana blanca en las nubes obscuras del Toro Boletin de los Observatorios de Tonantzintla y Tacubaya 3 35 Bibcode 1961BOTT 3 35H a b Landolt Arlo U 1968 A New Short Period Blue Variable The Astrophysical Journal 153 151 Bibcode 1968ApJ 153 151L doi 10 1086 149645 Koester D Chanmugam G 1990 Physics of white dwarf stars Reports on Progress in Physics 53 7 837 Bibcode 1990RPPh 53 837K doi 10 1088 0034 4885 53 7 001 S2CID 250915046 Dolez N et al 2006 Whole Earth telescope observations of the ZZ Ceti star HL Tau 76 Astronomy and Astrophysics 446 1 237 Bibcode 2006A amp A 446 237D doi 10 1051 0004 6361 20053149 Greenstein Jesse L October 1969 The Lowell Suspect White Dwarfs Astrophysical Journal 158 281 Bibcode 1969ApJ 158 281G doi 10 1086 150191 Kukarkin B V et al October 1970 57th Name List of Variable Stars Information Bulletin on Variable Stars 480 1 1 Bibcode 1970IBVS 480 1K Chen Y H Shu H January 2021 Asteroseismology of the DAV star R808 Monthly Notices of the Royal Astronomical Society 500 4 4703 4709 arXiv 2011 06918 Bibcode 2021MNRAS 500 4703C doi 10 1093 mnras staa3572 Retrieved from https en wikipedia org w index php title HL Tau 76 amp oldid 1169949519, wikipedia, wiki, book, books, library,

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