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CK Vulpeculae information


CK Vulpeculae

CK Vulpeculae taken by ALMA.[1]
Credit: ALMA (ESO/NAOJ/NRAO)/S. P. S. Eyres
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Vulpecula
Right ascension 19h 47m 38.0s[2]
Declination +27° 18′ 48″[2]
Apparent magnitude (V) max 2.6[2]
Characteristics
B−V color index 0.7[3]
Variable type unknown[3]
Astrometry
Distance10000+3000
−2000
[4] ly
(3200+900
−600
[4] pc)
Details
Luminosity0.9[3] L
Temperature14,000 – 100,000[3] K
Other designations
CK Vulpeculae, CK Vul, Nova Vul 1670, HR 7539, 11 Vul[5]
Database references
SIMBADdata

CK Vulpeculae (also Nova Vulpeculae 1670) is an object whose exact nature is unknown.[4] It was once considered to be the oldest reliably-documented nova. It consists of a compact central object surrounded by a bipolar nebula.

Models suggest CK Vulpeculae may not be a classic nova; rather it may be classified as a luminous red nova which is the result of two main sequence stars colliding and merging. A 2018 study found it was most likely the result of an unusual collision of a white dwarf and a brown dwarf. A 2020 article ruled out this proposed mechanism and proposes that CK Vulpeculae is an intermediate luminosity optical transient, i.e. an object in the luminosity gap between supernovae and novae.[4]

  1. ^ "Through the Hourglass". www.eso.org. Retrieved 8 October 2018.
  2. ^ a b c Cite error: The named reference downes was invoked but never defined (see the help page).
  3. ^ a b c d Cite error: The named reference Evans2016 was invoked but never defined (see the help page).
  4. ^ a b c d Cite error: The named reference bane was invoked but never defined (see the help page).
  5. ^ Morton, Wagman (2003). Lost Stars. Blacksburg, Virginia: McDonald and Woodward. p. 494. ISBN 978-0-939923-78-6.

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CK Vulpeculae

Last Update:

CK Vulpeculae (also Nova Vulpeculae 1670) is an object whose exact nature is unknown. It was once considered to be the oldest reliably-documented nova...

Word Count : 1417

Brown dwarf

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could also exist brown dwarfs that merged with white dwarfs. The nova CK Vulpeculae might be a result of such a white dwarf–brown dwarf merger. Substellar...

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Flamsteed designation

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into his catalog as a star called "34 Tauri". 11 Vulpeculae was a nova, now known as CK Vulpeculae. Many of them were caused by arithmetic errors made...

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Intermediate luminosity optical transient

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widespread use, it has begun to be applied to some objects like KjPn 8 and CK Vulpeculae for which no transient event has been observed, but which may have been...

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List of novae in the Milky Way galaxy

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Year Nova Maximum brightness 1612 04550 Leonis +4.0 1670 CK Vulpeculae +2.6 1673 03846 Puppis +3.0 1678 V529 Orionis +6 1783 WY Sagittae +5.4 1848 V841...

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V1309 Scorpii

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has already been used to try to explain the mysterious outburst of CK Vulpeculae in 1670–1672 that has puzzled scientists for centuries. Past spectroscopic...

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Anthelme Voituret

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star Mira. He is credited with being the first to observe the Nova 1670 Vulpeculae, the first ordinary nova discovered in modern times. In 1681, he published...

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WY Sagittae

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identified the post-nova star), with only CK Vulpeculae being older. But Naylor et al. argue that CK Vulpeculae is not a nova, and WY Sagittae is the oldest...

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V605 Aquilae

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Harrison, Thomas E. (1996). "A Near-Infrared Survey of Old Novae--II. CK Vulpeculae and V605 Aquilae". Publications of the Astronomical Society of the Pacific...

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List of largest stars

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Modelling VLTI/GRAVITY and MATISSE observations of AH Sco, KW Sgr, V602 Car, CK Car and V460 Car". Astronomy & Astrophysics. 683: A19. arXiv:2312.12521. doi:10...

Word Count : 10487

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