TU Andromedae
TU Andromedae (TU And) is a variable star of the Mira type in the constellation Andromeda. Like all the stars of this kind, TU And is a cool asymptotic giant branch star. It has a spectral type M5e. The period is stable at 316.8 days. The peak brightness, however, is different in each cycle and reach a peak magnitude (mv) of 7.5.[2]
{{Starbox astrometry
Observation data Epoch J2000 Equinox J2000 | ||||||
---|---|---|---|---|---|---|
Constellation | Andromeda | |||||
Right ascension | 00h 32m 22.72764s[1] | |||||
Declination | +26° 01′ 45.90759″[1] | |||||
Apparent magnitude (V) | 7.5 – 13.5[2] | |||||
Characteristics | ||||||
Spectral type | M5e[2] | |||||
B−V color index | 0.96[3] | |||||
Variable type | Mira[2] | |||||
radial_v= | prop_mo_ra= −6.877±0.206[1] | -2.278|0.139}}[1] | parallax= 1.5775 | p_error= 0.1124 | parallax_footnote = [1] | absmag_v=
}} |
Details | ||||||
Mass | 1.1[4] M☉ | |||||
Luminosity | 5,200 - 5,400[4] L☉ | |||||
Other designations | ||||||
HD 2890, HIP 2546, 2MASS J00322275+2601459 | ||||||
Database references | ||||||
SIMBAD | data |
The modelled properties of TU Andromedae at maximum brightness are not in agreement with available models of Mira stars (which work for Mira itself). It's uncertain if the problem is in the measured parameters of the star or in imperfections of the models.[4]
References
- 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.
- TU And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Accessed on line 2009-06-30.
- Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000), "The Tycho-2 catalogue of the 2.5 million brightest stars", Astronomy & Astrophysics, 355: L27–L30, Bibcode:2000A&A...355L..27H.
- Hillen, M.; Verhoelst, T.; Degroote, P.; Acke, B.; van Winckel, H. (2012), "The dynamic atmospheres of Mira stars: comparing the CODEX models to PTI time series of TU Andromedae", Astronomy & Astrophysics, 538, Bibcode:2012A&A...538L...6H, doi:10.1051/0004-6361/201118653.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.