Rise and fall of the dust shell of the classical nova V339 Delphini
We present infrared spectroscopy of the classical nova V339 Delphini, obtained over a $\sim2$ year period. The infrared emission lines were initially symmetrical, with HWHM velocities of 525 km s$^{-1}$. In later ($t\gtrsim77
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
20 December 2016
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| In: |
Arxiv
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| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1612.06241
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| Verfasserangaben: | A. Evans, D.P.K. Banerjee, R.D. Gehrz, V. Joshi, N.M. Ashok, V.a.R.M. Ribeiro, M.J. Darnley, C.E. Woodward, D. Sand, G.H. Marion, T.R. Diamond, S.P.S. Eyres, R.M. Wagner, L.A. Helton, S. Starrfield, D.P. Shenoy, J. Krautter, W.D. Vacca, M.T. Rushton |
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| 520 | |a We present infrared spectroscopy of the classical nova V339 Delphini, obtained over a $\sim2$ year period. The infrared emission lines were initially symmetrical, with HWHM velocities of 525 km s$^{-1}$. In later ($t\gtrsim77 | ||
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