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Q Cygni

From Wikipedia, the free encyclopedia
1876 Nova in the constellation Cygnus
Q Cygni
Location of Q Cygni (circled in red)
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus
Right ascension21h 41m 43.928s[1]
Declination42° 50′ 29.04″[1]
Apparent magnitude (V)3.0 - 15.6[2]
Characteristics
Spectral typeK5[3]
Variable typeNova[2]
Astrometry
Parallax (π)0.729±0.024 mas[4]
Distance1372+51
−42
[4](741[5] - 3,300[6]) pc
Absolute magnitude (MV)−9.1 -+2.9[4]
Details
White dwarf
Mass0.8[5] M
Surface gravity (log g)8.5[5] cgs
Temperature31,000[5] K
secondary
Mass0.6[3] M
Other designations
Nova Cygni 1876,HR 8296,BD+42°4182a,AAVSO 2137+42,2MASS J21414393+4250290,Gaia DR2 1966874711229398656
Database references
SIMBADdata

Q Cygni (Q Cyg), is astar located in theconstellation Cygnus. It is also known asNova Cygni 1876, and has the designationNGC 7114, andHR 8296. Nova Cygni is located in the northwestern portion of Cygnus along the border withLacerta.

One of the earliestnovae recorded,[6] Q Cygni was discovered by astronomerJohann Friedrich Julius Schmidt on November 24, 1876.[7] The star had undergone a nova, brightening to about 3rdmagnitude and remaining as bright for four days.[6]

The system is termed acataclysmic variable,[3] composed of awhite dwarf in closeorbit with another star that orbit each other every 10 hours. The white dwarf is surrounded by anaccretion disc, which blazes much brighter than the star it circles. The system has been estimated to be 740 ± 11 parsecs distant.[5] The secondary star has been estimated to be around 0.6 times as massive as the Sun, making it an orange dwarf of spectral type K5.[3] Also known as a donor star, the secondary supplies mass to the white dwarf via its accretion disc.[3]

A small nebulous disc was reported around the nova and this led to it being listed in theNew General Catalogue as a possibleplanetary nebula. Nonebulosity is visible in modern observations and theRevised New General Catalogue lists this as a"non-existent" object.[8]

Thelight curve of Q Cygni. The red points are from a table published by Schmidt, and the blue points were measured from a plot published by Lockyer.[9][10]

References

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  1. ^abBrown, 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. Gaia DR2 record for this source atVizieR.
  2. ^abSamus, 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.
  3. ^abcdePeters, Christopher S.; Thorstensen, John R. (2006)."Spectroscopy of Five Old Novae: New or Refined Orbital Periods".The Publications of the Astronomical Society of the Pacific.118 (843): 687.Bibcode:2006PASP..118..687P.doi:10.1086/504641.
  4. ^abcSchaefer, Bradley E. (2018)."The distances to Novae as seen by Gaia".Monthly Notices of the Royal Astronomical Society.481 (3):3033–3051.arXiv:1809.00180.Bibcode:2018MNRAS.481.3033S.doi:10.1093/mnras/sty2388.S2CID 118925493.
  5. ^abcdeKolobow, Craig; Sion, Edward (2011). "The Amazing Old Nova Q Cygni: A Far-Ultraviolet Synthetic Spectral Analysis".Publications of the Astronomical Society of the Pacific.123 (906):892–94.arXiv:1106.1562.Bibcode:2011PASP..123..892K.doi:10.1086/661235.S2CID 118737622.
  6. ^abcKafka, S.; Tappert, C.; Honeycutt, R. K.; Bianchini, A. (2003)."Spectroscopic Study of Q Cygni: Surprises from an Old Nova".The Astronomical Journal.126 (3):1472–82.Bibcode:2003AJ....126.1472K.doi:10.1086/377020.
  7. ^Duerbeck, Hilmar W. (March 1987). "A Reference Catalogue and Atlas of Galactic Novae".Space Science Reviews.45 (1–2):1–14.Bibcode:1987SSRv...45....1D.doi:10.1007/BF00187826.S2CID 115854775.
  8. ^"NGC 7000 - 7840". Archived fromthe original on 2016-09-16. Retrieved2016-09-07.
  9. ^Schmidt, Johann Friedrich Julius (January 1877). "Über den neuen Stern im Schwan".Astronomische Nachrichten.89 (3): 41.Bibcode:1877AN.....89...41S.doi:10.1002/asna.18770890304.
  10. ^Lockyer, J. Norman (January 1891)."On the Causes which Produce the Phenomena of New Stars".Philosophical Transactions of the Royal Society of London, Series A.182:397–448.Bibcode:1891RSPTA.182..397L.doi:10.1098/rsta.1891.0011.

External links

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