T Boötis

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Location of T Boötes (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Boötes
Right ascension 14h 14m 07.00s
Declination +19° 04′ 00.0″
Apparent magnitude (V) 9.7-<20.4
Characteristics
Variable type N (Nova)
Other designations
AAVSO 1409+19, BD+19 2768
Database references
SIMBADdata

T Boötis is believed to have been a nova. It was observed by only one person, Joseph Baxendell on 9, 11 and 22 April 1860, but has not been seen since. It is located less than half a degree from Arcturus in the constellation Boötes and was at magnitude 9.75 when first seen, and magnitude 12.8 when last seen. Other astronomers, including Friedrich Winnecke, Edward Charles Pickering, Ernst Hartwig and Ernst Zinner looked for a star in this location without success.

Despite being usually referred to as a nova, it had characteristics that set it apart from other novae - an amplitude of at least 7 magnitudes, an unusually rapid decline in brightness and a location unusually far from the Galactic plane. Joseph Ashbrook suggested in 1953 that it may be a recurrent nova which has been observed only once.

References

  1. ^ a b c d "VSX: Detail for T Boo". The International Variable Star Index. AAVSO. Archived from the original on 28 April 2017. Retrieved 16 May 2015.
  2. ^ a b Baxendell, Joseph (1861). "On the Three New Variable Stars, T Bootis, T. Serpentis, and S Delphini". Monthly Notices of the Royal Astronomical Society. 21 (3). Smithsonian Astrophysical Observatory: 68. Bibcode:1861MNRAS..21...68B. doi:10.1093/mnras/21.3.68.
  3. ^ a b Burnham, Robert (1978). Burnham's Celestial Handbook Volume 1. Dover. p. 311. ISBN 978-0-486-31902-5.
  4. ^ Ashbrook, Joseph (1953). "Notes on Four Novae". The Astronomical Journal. 58. Smithsonian Astrophysical Observatory: 175. Bibcode:1953AJ.....58..175F. doi:10.1086/106846. Archived from the original on 27 May 2024. Retrieved 16 May 2015.


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