The early infrared temporal development of nova delphini 2013 (v339 del) observed with the stratospheric observatory for infrared astronomy (sofia) and from the ground

R. D. Gehrz; L. A. Helton; D. P. Shenoy; D. P. K. Banerjee; C. E. Woodward; W. D. Vacca; D. A. Dykhoff; N. M. Ashok; A. C. Cass; R. L. Carlon; D. T. Corgan; S. P.S. Eyres; V. Joshi; Luke D. Keller; J. Krautter; T. Liimets; M. T. Rushton; S. Starrfield; A. Evans

doi:10.1088/0004-637X/812/2/132

The early infrared temporal development of nova delphini 2013 (v339 del) observed with the stratospheric observatory for infrared astronomy (sofia) and from the ground

R. D. Gehrz, L. A. Helton, D. P. Shenoy, D. P. K. Banerjee, C. E. Woodward, W. D. Vacca, D. A. Dykhoff, N. M. Ashok, A. C. Cass, R. L. Carlon, D. T. Corgan, S. P.S. Eyres, V. Joshi, Luke D. Keller, J. Krautter, T. Liimets, M. T. Rushton, S. Starrfield, A. Evans

Faculty of Computing, Engineering and Science

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Abstract

We present ground-based infrared photometry, JHK spectroscopy, and 5-28 μm SOFIA FORCAST spectroscopy documenting the early temporal development of Nova Delphini 2013 (V339 Del). We derive a distance of ∼4.5 kpc using data available from the early expansion of the fireball. This distance gives an outburst luminosity of ∼8.3 × 10⁵ making V339 Del the most luminous CO nova on record. Our data provide new constraints on the ejected gas mass and the dust yield in fast CO novae. The ejected gas mass as estimated by the cutoff wavelength during the free-free emission phase is ∼7.5 × 10^-5 There is evidence for the formation of ∼1.2(±0.4) × 10^-7 of dust about 102 days after outburst. The gas to dust ratio of ∼470/1-940/1 implies that dust production was much less efficient in V339 Del than is the case for most CO novae.

Original language	English
Article number	132
Journal	The Astrophysical Journal
Volume	812
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/812/2/132
Publication status	Published - 20 Oct 2015

Keywords

circumstellar matter
infrared: Stars
novae, cataclysmic variables
stars: individual (V339 Del)
stars: winds, outflows

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Gehrz, R. D., Helton, L. A., Shenoy, D. P., Banerjee, D. P. K., Woodward, C. E., Vacca, W. D., Dykhoff, D. A., Ashok, N. M., Cass, A. C., Carlon, R. L., Corgan, D. T., Eyres, S. P. S., Joshi, V., Keller, L. D., Krautter, J., Liimets, T., Rushton, M. T., Starrfield, S., & Evans, A. (2015). The early infrared temporal development of nova delphini 2013 (v339 del) observed with the stratospheric observatory for infrared astronomy (sofia) and from the ground. The Astrophysical Journal, 812(2), Article 132. https://doi.org/10.1088/0004-637X/812/2/132

@article{7559125a25ec40a5931f6effcb925501,

title = "The early infrared temporal development of nova delphini 2013 (v339 del) observed with the stratospheric observatory for infrared astronomy (sofia) and from the ground",

abstract = "We present ground-based infrared photometry, JHK spectroscopy, and 5-28 μm SOFIA FORCAST spectroscopy documenting the early temporal development of Nova Delphini 2013 (V339 Del). We derive a distance of ∼4.5 kpc using data available from the early expansion of the fireball. This distance gives an outburst luminosity of ∼8.3 × 105 making V339 Del the most luminous CO nova on record. Our data provide new constraints on the ejected gas mass and the dust yield in fast CO novae. The ejected gas mass as estimated by the cutoff wavelength during the free-free emission phase is ∼7.5 × 10-5 There is evidence for the formation of ∼1.2(±0.4) × 10-7 of dust about 102 days after outburst. The gas to dust ratio of ∼470/1-940/1 implies that dust production was much less efficient in V339 Del than is the case for most CO novae.",

keywords = "circumstellar matter, infrared: Stars, novae, cataclysmic variables, stars: individual (V339 Del), stars: winds, outflows",

author = "Gehrz, {R. D.} and Helton, {L. A.} and Shenoy, {D. P.} and Banerjee, {D. P. K.} and Woodward, {C. E.} and Vacca, {W. D.} and Dykhoff, {D. A.} and Ashok, {N. M.} and Cass, {A. C.} and Carlon, {R. L.} and Corgan, {D. T.} and Eyres, {S. P.S.} and V. Joshi and Keller, {Luke D.} and J. Krautter and T. Liimets and Rushton, {M. T.} and S. Starrfield and A. Evans",

year = "2015",

month = oct,

day = "20",

doi = "10.1088/0004-637X/812/2/132",

language = "English",

volume = "812",

journal = "The Astrophysical Journal",

issn = "0004-637X",

publisher = "University of Chicago Press",

number = "2",

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Gehrz, RD, Helton, LA, Shenoy, DP, Banerjee, DPK, Woodward, CE, Vacca, WD, Dykhoff, DA, Ashok, NM, Cass, AC, Carlon, RL, Corgan, DT, Eyres, SPS, Joshi, V, Keller, LD, Krautter, J, Liimets, T, Rushton, MT, Starrfield, S & Evans, A 2015, 'The early infrared temporal development of nova delphini 2013 (v339 del) observed with the stratospheric observatory for infrared astronomy (sofia) and from the ground', The Astrophysical Journal, vol. 812, no. 2, 132. https://doi.org/10.1088/0004-637X/812/2/132

TY - JOUR

T1 - The early infrared temporal development of nova delphini 2013 (v339 del) observed with the stratospheric observatory for infrared astronomy (sofia) and from the ground

AU - Gehrz, R. D.

AU - Helton, L. A.

AU - Shenoy, D. P.

AU - Banerjee, D. P. K.

AU - Woodward, C. E.

AU - Vacca, W. D.

AU - Dykhoff, D. A.

AU - Ashok, N. M.

AU - Cass, A. C.

AU - Carlon, R. L.

AU - Corgan, D. T.

AU - Eyres, S. P.S.

AU - Joshi, V.

AU - Keller, Luke D.

AU - Krautter, J.

AU - Liimets, T.

AU - Rushton, M. T.

AU - Starrfield, S.

AU - Evans, A.

PY - 2015/10/20

Y1 - 2015/10/20

N2 - We present ground-based infrared photometry, JHK spectroscopy, and 5-28 μm SOFIA FORCAST spectroscopy documenting the early temporal development of Nova Delphini 2013 (V339 Del). We derive a distance of ∼4.5 kpc using data available from the early expansion of the fireball. This distance gives an outburst luminosity of ∼8.3 × 105 making V339 Del the most luminous CO nova on record. Our data provide new constraints on the ejected gas mass and the dust yield in fast CO novae. The ejected gas mass as estimated by the cutoff wavelength during the free-free emission phase is ∼7.5 × 10-5 There is evidence for the formation of ∼1.2(±0.4) × 10-7 of dust about 102 days after outburst. The gas to dust ratio of ∼470/1-940/1 implies that dust production was much less efficient in V339 Del than is the case for most CO novae.

AB - We present ground-based infrared photometry, JHK spectroscopy, and 5-28 μm SOFIA FORCAST spectroscopy documenting the early temporal development of Nova Delphini 2013 (V339 Del). We derive a distance of ∼4.5 kpc using data available from the early expansion of the fireball. This distance gives an outburst luminosity of ∼8.3 × 105 making V339 Del the most luminous CO nova on record. Our data provide new constraints on the ejected gas mass and the dust yield in fast CO novae. The ejected gas mass as estimated by the cutoff wavelength during the free-free emission phase is ∼7.5 × 10-5 There is evidence for the formation of ∼1.2(±0.4) × 10-7 of dust about 102 days after outburst. The gas to dust ratio of ∼470/1-940/1 implies that dust production was much less efficient in V339 Del than is the case for most CO novae.

KW - circumstellar matter

KW - infrared: Stars

KW - novae, cataclysmic variables

KW - stars: individual (V339 Del)

KW - stars: winds, outflows

U2 - 10.1088/0004-637X/812/2/132

DO - 10.1088/0004-637X/812/2/132

M3 - Article

AN - SCOPUS:84946064725

SN - 0004-637X

VL - 812

JO - The Astrophysical Journal

JF - The Astrophysical Journal

IS - 2

M1 - 132

ER -

The early infrared temporal development of nova delphini 2013 (v339 del) observed with the stratospheric observatory for infrared astronomy (sofia) and from the ground

Abstract

Keywords

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