CK Vul: a smorgasbord of hydrocarbons rules out a 1670 nova (and much else besides)

R. D. Gehrz; C. E. Woodward; P. J. Sarre; J. T. van Loon; L. A. Helton; S. Starrfield; S. P. S. Eyres; A. Evans

doi:10.1093/mnras/stw352

CK Vul: a smorgasbord of hydrocarbons rules out a 1670 nova (and much else besides)

R. D. Gehrz, C. E. Woodward, P. J. Sarre, J. T. van Loon, L. A. Helton, S. Starrfield, S. P. S. Eyres, A. Evans^*

^*Awdur cyfatebol y gwaith hwn

Allbwn ymchwil: Cyfraniad at gyfnodolyn › Erthygl › adolygiad gan gymheiriaid

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We present observations of CK Vul obtained with the Spitzer Space Telescope. The infrared spectrum reveals a warm dust continuum with nebular, molecular hydrogen and HCN lines superimposed, together with the 'Unidentified Infrared' features. The nebular lines are consistent with emission by a low-density gas. We conclude that the Spitzer data, combined with other information, are incompatible with CK Vul being a classical nova remnant in 'hibernation' after the event of 1670, a 'very late thermal pulse', a 'Luminous Red Variable', such as V838 Mon, or a 'diffusion-induced nova'. The true nature of CK Vul remains a mystery.

Iaith wreiddiol	Saesneg
Tudalennau (o-i)	2871-2876
Nifer y tudalennau	6
Cyfnodolyn	Monthly Notices of the Royal Astronomical Society
Cyfrol	457
Rhif cyhoeddi	3
Dyddiad ar-lein cynnar	17 Chwef 2016
Dynodwyr Gwrthrych Digidol (DOIs)	https://doi.org/10.1093/mnras/stw352
Statws	E-gyhoeddi cyn argraffu - 17 Chwef 2016
Cyhoeddwyd yn allanol	Ie

Mynediad at Ddogfen

10.1093/mnras/stw352Trwydded: CC BY-NC-ND

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title = "CK Vul: a smorgasbord of hydrocarbons rules out a 1670 nova (and much else besides)",

abstract = "We present observations of CK Vul obtained with the Spitzer Space Telescope. The infrared spectrum reveals a warm dust continuum with nebular, molecular hydrogen and HCN lines superimposed, together with the 'Unidentified Infrared' features. The nebular lines are consistent with emission by a low-density gas. We conclude that the Spitzer data, combined with other information, are incompatible with CK Vul being a classical nova remnant in 'hibernation' after the event of 1670, a 'very late thermal pulse', a 'Luminous Red Variable', such as V838 Mon, or a 'diffusion-induced nova'. The true nature of CK Vul remains a mystery.",

keywords = "circumstellar matter, stars: individual: CK Vul, ISM: molecules, infrared: stars, SPITZER-SPACE-TELESCOPE, PLANETARY-NEBULAE, CLASSICAL NOVAE, DUST, EMISSION, EVOLUTION, MOLECULES, FEATURES, STARS, PAHS",

author = "Gehrz, {R. D.} and Woodward, {C. E.} and Sarre, {P. J.} and {van Loon}, {J. T.} and Helton, {L. A.} and S. Starrfield and Eyres, {S. P. S.} and A. Evans",

year = "2016",

month = feb,

day = "17",

doi = "10.1093/mnras/stw352",

language = "English",

volume = "457",

pages = "2871--2876",

journal = "Monthly Notices of the Royal Astronomical Society",

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publisher = "Oxford University Press",

number = "3",

}

TY - JOUR

T1 - CK Vul

T2 - a smorgasbord of hydrocarbons rules out a 1670 nova (and much else besides)

AU - Gehrz, R. D.

AU - Woodward, C. E.

AU - Sarre, P. J.

AU - van Loon, J. T.

AU - Helton, L. A.

AU - Starrfield, S.

AU - Eyres, S. P. S.

AU - Evans, A.

PY - 2016/2/17

Y1 - 2016/2/17

N2 - We present observations of CK Vul obtained with the Spitzer Space Telescope. The infrared spectrum reveals a warm dust continuum with nebular, molecular hydrogen and HCN lines superimposed, together with the 'Unidentified Infrared' features. The nebular lines are consistent with emission by a low-density gas. We conclude that the Spitzer data, combined with other information, are incompatible with CK Vul being a classical nova remnant in 'hibernation' after the event of 1670, a 'very late thermal pulse', a 'Luminous Red Variable', such as V838 Mon, or a 'diffusion-induced nova'. The true nature of CK Vul remains a mystery.

AB - We present observations of CK Vul obtained with the Spitzer Space Telescope. The infrared spectrum reveals a warm dust continuum with nebular, molecular hydrogen and HCN lines superimposed, together with the 'Unidentified Infrared' features. The nebular lines are consistent with emission by a low-density gas. We conclude that the Spitzer data, combined with other information, are incompatible with CK Vul being a classical nova remnant in 'hibernation' after the event of 1670, a 'very late thermal pulse', a 'Luminous Red Variable', such as V838 Mon, or a 'diffusion-induced nova'. The true nature of CK Vul remains a mystery.

KW - circumstellar matter

KW - stars: individual: CK Vul

KW - ISM: molecules

KW - infrared: stars

KW - SPITZER-SPACE-TELESCOPE

KW - PLANETARY-NEBULAE

KW - CLASSICAL NOVAE

KW - DUST

KW - EMISSION

KW - EVOLUTION

KW - MOLECULES

KW - FEATURES

KW - STARS

KW - PAHS

U2 - 10.1093/mnras/stw352

DO - 10.1093/mnras/stw352

M3 - Article

SN - 0035-8711

VL - 457

SP - 2871

EP - 2876

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

CK Vul: a smorgasbord of hydrocarbons rules out a 1670 nova (and much else besides)

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