BP Tauri

BP Tauri

A light curve for BP Tauri, plotted from TESS data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 04h 19m 15.8343s[2]
Declination +29° 06′ 26.9295″[2]
Apparent magnitude (V) 12.12
Characteristics
Evolutionary stage pre-main-sequence star
Spectral type K5
Apparent magnitude (G) 11.460[3]
Variable type T Tau
Astrometry
Radial velocity (Rv)15.76±0.13 km/s
Proper motion (μ) RA: 8.889[3] mas/yr
Dec.: -26.011[3] mas/yr
Parallax (π)7.8494 ± 0.0362 mas[3]
Distance416 ± 2 ly
(127.4 ± 0.6 pc)
Details
Mass1.24+0.25
−0.32
[4] M
Radius2.0[5] R
Luminosity0.93[5] L
Surface gravity (log g)4.32±0.14[6] cgs
Temperature3640+94
−92
[6] K
Rotational velocity (v sin i)11.4+0.25
−0.55
[6] km/s
Age6±4[4] Myr
Other designations
Gaia DR2 164832740220756608, HD 281934, HIP 20160, TYC 1827-554-1, GSC 01827-00554, 2MASS J04191583+2906269
Database references
SIMBADdata

BP Tauri is a young T Tauri star in the constellation of Taurus about 416 light years away, belonging to the Taurus Molecular Cloud.

  1. ^ Cite error: The named reference MAST was invoked but never defined (see the help page).
  2. ^ a b Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  3. ^ a b c d Cite error: The named reference EDR3 was invoked but never defined (see the help page).
  4. ^ a b Simon, M.; Dutrey, A.; Guilloteau, S. (2000), "Dynamical Masses of T Tauri Stars and Calibration of Pre–Main-Sequence Evolution", The Astrophysical Journal, 545 (2): 1034–1043, arXiv:astro-ph/0008370, Bibcode:2000ApJ...545.1034S, doi:10.1086/317838, S2CID 18064837
  5. ^ a b Errico, L.; Lamzin, S. A.; Vittone, A. A. (2001), "UV spectra of T Tauri stars from the HST and IUE satellites: BP Tau", Astronomy & Astrophysics, 377 (2): 557–565, Bibcode:2001A&A...377..557E, doi:10.1051/0004-6361:20011108
  6. ^ a b c Flores, C.; Connelley, M. S.; Reipurth, B.; Boogert, A. (2019), "Measuring the Magnetic Field of Young Stars Using iSHELL Observations: BP Tau and V347 Aur", The Astrophysical Journal, 882 (2): 75, arXiv:1908.08583, Bibcode:2019ApJ...882...75F, doi:10.3847/1538-4357/ab35d4, S2CID 201645503