R Aquarii

From Wikipedia, the free encyclopedia
Jump to: navigation, search
R Aquarii
R Aquarii.jpg
R Aquarii
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 23h 43m 49.4616s
Declination −15° 17′ 04.202″
Apparent magnitude (V) 5.72 - 12.4 [1]
Characteristics
Spectral type M7IIIpev
U−B color index 0.32
B−V color index 1.58
Variable type Mira Cet
Astrometry
Radial velocity (Rv) -22 km/s
Proper motion (μ) RA: 32.98 mas/yr
Dec.: -32.61 mas/yr
Parallax (π) 5.07 ± 3.15 mas
Distance approx. 600 ly
(approx. 200 pc)
Absolute magnitude (MV) -6.87 - 0.33 [2]
Details
Mass 1.5, 0.5[3] M
Radius 430, 0.014 [3] R
Luminosity 50,000 - 1.6 [3] L
Other designations
BD-16 6352, HD 222800, HIP 117054, HR 8992, SAO 165849.
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

R Aquarii (R Aqr) is a variable star in the constellation Aquarius.

R Aquarii is a symbiotic star believed to contain a white dwarf and a Mira-type variable in a binary system. The orbital period is approximately 44 years.[4] The main Mira-type star is a red giant, and varies in brightness by a factor of several hundred and with a period of slightly more than a year; this variability was discovered by Karl Ludwig Harding in 1810. It has a distance of about 200 parsec, and is one of the nearest symbiotic stars and a well known jet source.[5]

By its gravitational pull, the white dwarf draws in material from the red giant and occasionally ejects some of the surplus in weird loops to form the nebula seen in the linked image.[6] The whole system appears reddened because it is situated in a very dusty region of space, and its blue light is absorbed before reaching us.

The nebula around R Aquarii is also known as Cederblad 211. According to Tom Polakis,[7] as of 1998 no one had succeeded to observe this challenging object visually. It is possible that the nebula is the remnant of a nova-like outburst, which may have been observed by Japanese astronomers, in the year 930 AD.

References[edit]

  1. ^ http://www.sai.msu.su/gcvs/gcvs/index.htm
  2. ^ ibid
  3. ^ a b c M. Gromadzki and J. Miko¿ajewska (April 2009). "The spectroscopic orbit and the geometry of R Aquarii". Astronomy & Astrophysics 495 (4): 931–936. arXiv:0804.4139. Bibcode:2009A&A...495..931G. doi:10.1051/0004-6361:200810052. 
  4. ^ <Gromadzki and Mikolajewska (2009). "The spectroscopic orbit and the geometry of R Aquarii". Astronomy & Astrophysics 495 (3): 931¿936. arXiv:0804.4139. Bibcode:2009A&A...495..931G. doi:10.1051/0004-6361:200810052. 
  5. ^ Stute, Matthias; Sahai, Raghvendra. "Hydrodynamical Simulations of the Jet in the Symbiotic Star MWC 560". The Astrophysical Journal. The American Astronomical Society. Retrieved 10 October 2011. 
  6. ^ "Aladin previewer". CDS. 
  7. ^ Polakis, Tom (Oct 1998). Astronomy 26 (10): 83. 

External links[edit]