XZ Tauri

XZ Tauri is a binary system approximately 460 light-years away in the constellation Taurus. The system consists of two T Tauri stars orbiting each other about 6 billion kilometers apart (roughly the same distance as Pluto is from the Sun). The system made news in 2000 when a superflare was observed in the system.

XZ Tauri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Taurus
Right ascension 04h 31m 40.08690s[1]
Declination +18° 13 56.6424[1]
Apparent magnitude (V) 11.00
Characteristics
Spectral type M2.0 + M3.5[2]
Astrometry
Distance460 ly
(140[3] pc)
Details[2]
A
Mass0.37 M
Radius1.1 R
Luminosity0.17 L
B
Mass0.29 M
Radius1.7 R
Luminosity0.31 L
Temperature3,550[3] K
Age4.6[3] Myr
Other designations
XZ Tau, GSC 01269-00171[4]
Database references
SIMBADdata

References

  1. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. Hartigan, Patrick; Kenyon, Scott J. (January 2003). "A Spectroscopic Survey of Subarcsecond Binaries in the Taurus-Auriga Dark Cloud with the Hubble Space Telescope". The Astrophysical Journal. 583 (1): 334–357. arXiv:astro-ph/0209608. Bibcode:2003ApJ...583..334H. doi:10.1086/345293.
  3. Osorio, Mayra; et al. (July 2016). "A Dwarf Transitional Protoplanetary Disk around XZ Tau B". The Astrophysical Journal Letters. 825 (1): 6. arXiv:1606.03118. Bibcode:2016ApJ...825L..10O. doi:10.3847/2041-8205/825/1/L10. L10.
  4. "XZ Tau". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-12-09.
  5. "Jets, bubbles, and bursts of light in Taurus". www.spacetelescope.org. ESA/Hubble. Retrieved 6 November 2014.
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