The shell of QU Vulpeculae at 2.2 microns, Hα, and 3.6 centimeters

J. Y. Shin; Robert D. Gehrz; Terry Jay Jones; Joachim Krautter; J. Heidt; R. M. Hjellming

doi:10.1086/300529

The shell of QU Vulpeculae at 2.2 microns, Hα, and 3.6 centimeters

J. Y. Shin, Robert D. Gehrz, Terry Jay Jones, Joachim Krautter, J. Heidt, R. M. Hjellming

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7 Scopus citations

Abstract

Observations of the classical nova QU Vul (1984) were carried out in the infrared, optical, and radio regimes between days 3791 and 4262 after discovery. For the first time a spatial extension of the shell around QU Vul could be unambiguously established from our IR and optical observations. At 2.2 μm, a shell size of about 0″.S was found, which corresponds to a linear diameter of (4.5 ± 0.4) × 10¹⁶ cm on day 4124 assuming QU Vul is 3.6 kpc distant. The mass of the shell is (4 ± 1.5) × 10^-4 M_⊙ with the assumption that a free-free emission process is the dominant emission mechanism in the shell. This shell mass is larger than found for any nova.

Original language	English (US)
Pages (from-to)	1966-1970
Number of pages	5
Journal	Astronomical Journal
Volume	116
Issue number	4
DOIs	https://doi.org/10.1086/300529
State	Published - Oct 1998

Keywords

Infrared radiation
Novae, cataclysmic variables
Radio continuum

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10.1086/300529

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title = "The shell of QU Vulpeculae at 2.2 microns, Hα, and 3.6 centimeters",

abstract = "Observations of the classical nova QU Vul (1984) were carried out in the infrared, optical, and radio regimes between days 3791 and 4262 after discovery. For the first time a spatial extension of the shell around QU Vul could be unambiguously established from our IR and optical observations. At 2.2 μm, a shell size of about 0″.S was found, which corresponds to a linear diameter of (4.5 ± 0.4) × 1016 cm on day 4124 assuming QU Vul is 3.6 kpc distant. The mass of the shell is (4 ± 1.5) × 10-4 M⊙ with the assumption that a free-free emission process is the dominant emission mechanism in the shell. This shell mass is larger than found for any nova.",

keywords = "Infrared radiation, Novae, cataclysmic variables, Radio continuum",

author = "Shin, {J. Y.} and Gehrz, {Robert D.} and Jones, {Terry Jay} and Joachim Krautter and J. Heidt and Hjellming, {R. M.}",

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T1 - The shell of QU Vulpeculae at 2.2 microns, Hα, and 3.6 centimeters

AU - Shin, J. Y.

AU - Gehrz, Robert D.

AU - Jones, Terry Jay

AU - Krautter, Joachim

AU - Heidt, J.

AU - Hjellming, R. M.

PY - 1998/10

Y1 - 1998/10

N2 - Observations of the classical nova QU Vul (1984) were carried out in the infrared, optical, and radio regimes between days 3791 and 4262 after discovery. For the first time a spatial extension of the shell around QU Vul could be unambiguously established from our IR and optical observations. At 2.2 μm, a shell size of about 0″.S was found, which corresponds to a linear diameter of (4.5 ± 0.4) × 1016 cm on day 4124 assuming QU Vul is 3.6 kpc distant. The mass of the shell is (4 ± 1.5) × 10-4 M⊙ with the assumption that a free-free emission process is the dominant emission mechanism in the shell. This shell mass is larger than found for any nova.

AB - Observations of the classical nova QU Vul (1984) were carried out in the infrared, optical, and radio regimes between days 3791 and 4262 after discovery. For the first time a spatial extension of the shell around QU Vul could be unambiguously established from our IR and optical observations. At 2.2 μm, a shell size of about 0″.S was found, which corresponds to a linear diameter of (4.5 ± 0.4) × 1016 cm on day 4124 assuming QU Vul is 3.6 kpc distant. The mass of the shell is (4 ± 1.5) × 10-4 M⊙ with the assumption that a free-free emission process is the dominant emission mechanism in the shell. This shell mass is larger than found for any nova.

KW - Infrared radiation

KW - Novae, cataclysmic variables

KW - Radio continuum

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JF - Astronomical Journal

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The shell of QU Vulpeculae at 2.2 microns, Hα, and 3.6 centimeters

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