HK Tauri

HK Tauri

A light curve for HK Tauri, adapted from Roggero et al. (2021)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
A
Right ascension 04h 31m 50.5716s[2]
Declination +24° 24′ 17.775″[2]
Apparent magnitude (V) 15.10
B
Right ascension 04h 31m 50.6002s[3]
Declination +24° 24′ 15.503″[3]
Characteristics
HK Tauri A
Evolutionary stage pre-main-sequence star
Spectral type M1.5[4]
Apparent magnitude (G) 14.106[2]
Variable type T Tau
HK Tauri B
Spectral type M2[4]
Apparent magnitude (G) 17.962[3]
Astrometry
HK Tauri A
Proper motion (μ) RA: 5.076[2] mas/yr
Dec.: −22.944[2] mas/yr
Parallax (π)7.6247 ± 0.0317 mas[2]
Distance428 ± 2 ly
(131.2 ± 0.5 pc)
HK Tauri B
Proper motion (μ) RA: 2.668[3] mas/yr
Dec.: −20.457[3] mas/yr
Parallax (π)7.780 ± 0.6322 mas[3]
Distance420 ± 30 ly
(130 ± 10 pc)
Position (relative to HK Tauri A)[4]
ComponentHK Tauri B
Angular distance2.32
Position angle170.4°
Projected separation309 AU
Details
A
Mass0.44+0.14
−0.11
[4] M
Luminosity0.56[5] L
Temperature3680±150[6] K
B
Mass0.37±0.2[4] M
Luminosity0.42[5] L
Temperature3550±150[6] K
Other designations
2MASS J04315056+2424180, WISE J043150.56+242417.6
HK Tauri A: Gaia EDR3 147847072275324416, Gaia DR2 147847072275324416
HK Tauri B: Gaia EDR3 147847072275766656, Gaia DR2 147847072274696704
Database references
SIMBADdata

HK Tauri is a young binary star system in the constellation of Taurus about 434 light-years away, belonging to the Taurus Molecular Cloud.

  1. ^ Cite error: The named reference Roggero was invoked but never defined (see the help page).
  2. ^ a b c d e f Cite error: The named reference EDR3 was invoked but never defined (see the help page).
  3. ^ a b c d e f Cite error: The named reference EDR3B was invoked but never defined (see the help page).
  4. ^ a b c d e Manara, C. F.; Tazzari, M.; Long, F.; Herczeg, G. J.; Lodato, G.; Rota, A. A.; Cazzoletti, P.; Van Der Plas, G.; Pinilla, P.; Dipierro, G.; Edwards, S.; Harsono, D.; Johnstone, D.; Liu, Y.; Menard, F.; Nisini, B.; Ragusa, E.; Boehler, Y.; Cabrit, S. (2019), "Observational constraints on dust disk sizes in tidally truncated protoplanetary disks in multiple systems in the Taurus region", Astronomy & Astrophysics, 628: A95, arXiv:1907.03846, Bibcode:2019A&A...628A..95M, doi:10.1051/0004-6361/201935964, S2CID 195847916
  5. ^ a b Akeson, Rachel L.; Jensen, Eric L. N.; Carpenter, John; Ricci, Luca; Laos, Stefan; Nogueira, Natasha F.; Suen-Lewis, Emma M. (2019), "Resolved Young Binary Systems and Their Disks", The Astrophysical Journal, 872 (2): 158, arXiv:1901.05029, Bibcode:2019ApJ...872..158A, doi:10.3847/1538-4357/aaff6a, S2CID 119332907
  6. ^ a b Simon, M.; Guilloteau, S.; Beck, Tracy L.; Chapillon, E.; Folco, E. Di; Dutrey, A.; Feiden, Gregory A.; Grosso, N.; Piétu, V.; Prato, L.; Schaefer, Gail H. (2019), "Masses and Implications for Ages of Low-mass Pre-main-sequence Stars in Taurus and Ophiuchus", The Astrophysical Journal, 884 (1): 42, arXiv:1908.10952, Bibcode:2019ApJ...884...42S, doi:10.3847/1538-4357/ab3e3b, S2CID 201668492