TU Muscae

TU Muscae

A light curve for TU Muscae, plotted from TESS data[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Musca
Right ascension 11h 31m 10.92470s[2]
Declination −65° 44′ 32.1019″[2]
Apparent magnitude (V) 8.307[3](8.17 - 8.75[4])
Characteristics
Spectral type O7V + O8V[5]
U−B color index −0.860[3]
B−V color index +0.047[3]
Variable type β Lyr[4]
Astrometry
Radial velocity (Rv)−4[6] km/s
Proper motion (μ) RA: −6.62[2] mas/yr
Dec.: −1.21[2] mas/yr
Parallax (π)0.02 ± 0.76 mas[2]
Orbit[5]
Period (P)1.387 days
Semi-major axis (a)17.34 R[7]
Eccentricity (e)0
Inclination (i)77.7°
Longitude of the node (Ω)3.137[6]°
Semi-amplitude (K1)
(primary)
214.5 km/s
Semi-amplitude (K2)
(secondary)
345.8 km/s
Details[5]
Primary
Mass16.8 M
Radius7.2 R
Luminosity105,000 L
Surface gravity (log g)4.05[7] cgs
Temperature35,000[6] K
secondary
Mass10.5 M
Radius5.7 R
Luminosity35,000 L
Surface gravity (log g)4.04[7] cgs
Temperature31,366[6] K
Other designations
TU Muscae, HIP 56196, HD 100213, BD−65°1101, 2MASS J11311091-6544322
Database references
SIMBADdata

TU Muscae, also known as HD100213, is an eclipsing binary star in the constellation Musca. Its apparent magnitude ranges from 8.17 to 8.75 over around 1.4 days.[4]

  1. ^ Cite error: The named reference MAST was invoked but never defined (see the help page).
  2. ^ a b c d e Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
  3. ^ a b c Maíz-Apellániz, Jesús; Walborn, Nolan R.; Galué, Héctor Á.; Wei, Lisa H. (2004). "A Galactic O Star Catalog". The Astrophysical Journal Supplement Series. 151 (1): 103–148. arXiv:astro-ph/0311196. Bibcode:2004ApJS..151..103M. doi:10.1086/381380. S2CID 118813863.
  4. ^ a b c Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  5. ^ a b c Cite error: The named reference penny08 was invoked but never defined (see the help page).
  6. ^ a b c d Cite error: The named reference terrell03 was invoked but never defined (see the help page).
  7. ^ a b c Palate, M.; Rauw, G. (2012). "Spectral modelling of circular massive binary systems. Towards an understanding of the Struve-Sahade effect?". Astronomy & Astrophysics. 537: A119. arXiv:1109.1103. Bibcode:2012A&A...537A.119P. doi:10.1051/0004-6361/201117520. S2CID 84840295.