TY Coronae Borealis

Variable white dwarf in the constellation Corona Borealis From Wikipedia, the free encyclopedia

TY Coronae Borealis, also known as Ross 808, is a white dwarf in the constellation Corona Borealis. It is 107 light-years distant from Earth,[2] and has a dim apparent magnitude of 14.4.[3]

Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
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) 14.435±0.018[3]
Characteristics
Evolutionary stage White dwarf
Spectral type DA4.4[4]
Variable type ZZ Ceti[5]
Astrometry
Proper motion (μ) RA: 101.113 mas/yr[2]
Dec.: −545.353 mas/yr[2]
Parallax (π)30.4668±0.0187 mas[2]
Distance107.05 ± 0.07 ly
(32.82 ± 0.02 pc)
Absolute magnitude (MV)+11.81[6]
Details
Mass0.593±0.028 to 0.615+0.024
−0.025
[3] M
Radius0.0131±0.0014[7] R
Luminosity(1.83±0.03)×10−3[8] L
Surface gravity (log g)8.194[9] cgs
Temperature11,000[9] K
Age447 (white dwarf stage)[6] Myr
Other designations
TY CrB, Ross 808, WD 1600+369, LTT 14769, NLTT 41782, 2MASS J16012317+3648351[4]
Database references
SIMBADdata
Close

It is a pulsating white dwarf of the DAV (ZZ Ceti) type. The variation in the blue band is of 0.14 magnitudes, over a period of 15 minutes.[5] It was confirmed as a variable star in 1976, and now has the variable-star designation TY Coronae Borealis.[10] Being of this variable class, it has been a target for asteroseismic analyses, in attempt to derive its physical properties such as mass, radius and gravity.[9][11][8] However, it seems estimations of the stellar mass derived for this star using asteroseismology had been overestimated.[3]

TY Coronae Borealis has around 0.6 times the mass of the Sun[3] and a tiny diameter of only 1.3% that of the Sun.[7] It is a dim star, with 0.2% of the Sun's luminosity.[8] It has an effective temperature of about 11,000 K,[9] have taken 450 million years to cool to its temperature. This is also its age as a white dwarf.[6]

References

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