RZ Pyxidis

RZ Pyxidis is eclipsing binary system in the constellation Pyxis, made up of two young stars less than 200,000 years old. Both are hot blue-white stars of spectral type B7V and are around 2.5 times the size of the Sun. One is around five times as luminous as the sun and the other around four times as luminous.[3] The system is classified as a Beta Lyrae variable, he apparent magnitude ranging from 8.83 to 9.72 over 0.66 days.[2]

RZ Pyxidis
Observation data
Epoch J2000      Equinox J2000
Constellation Pyxis
Right ascension  08h 52m 04.39659s[1]
Declination –27° 29′ 01.4808″[1]
Apparent magnitude (V) 8.83 - 9.72[2]
Characteristics
Spectral type B7V
Variable type Beta Lyrae variable
Astrometry
Radial velocity (Rv)+22.00 ± 7.4 km/s
Proper motion (μ) RA: –4.67[1] mas/yr
Dec.: 4.61[1] mas/yr
Parallax (π)2.68 ± 1.67[1] mas
Distanceapprox. 1,200 ly
(approx. 400 pc)
Other designations
RZ Pyxidis, CD−27° 6009, HD 75920, HIP 43541, SAO 176601.
Database references
SIMBADdata

References
  1. van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–64, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357
  2. Watson, Christopher (4 January 2010). "RZ Pyxidis". The International Variable Star Index. American Association of Variable Star Observers. Retrieved 31 July 2015.
  3. Bell, S. A.; Malcolm, G. J. (1987). "RZ Pyxidis – an early-type marginal contact binary". Monthly Notices of the Royal Astronomical Society. 227: 481–500. Bibcode:1987MNRAS.227..481B. doi:10.1093/mnras/227.2.481. ISSN 0035-8711.


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