D2 Article in a professional compilation book
Spectroscopic classification of AT 2019sxc as a nova in M31 #13228
Authors: Williams SC, Darnley MJ, Healy MW, Murphy-Glaysher FJ, Ransome CL
Publisher: R. E. Rutledge
Publication year: 2019
Book title : Astronomer’s telegram
Journal name in source: The Astronomer's Telegram
Series title: Astronomer’s telegram
Number in series: 13228
Web address : https://www.astronomerstelegram.org/?read=13228
Abstract
We obtained a spectrum of the transient AT 2019sxc (see also ATel #13207) with the SPRAT spectrograph (resolution R 350; Piascik et al. 2014) on the 2-m Liverpool Telescope (LT; Steele et al. 2004) on 2019 Oct 23.93 UT. The spectrum shows strong Balmer emission lines (H & alpha;, H & beta;, H & gamma;, H & delta;), along with numerous Fe II emission lines, including those of the 27, 28, 37, 38, 42, 48, 49 and 74 multiplets.
We obtained a spectrum of the transient AT 2019sxc (see also ATel #13207) with the SPRAT spectrograph (resolution R 350; Piascik et al. 2014) on the 2-m Liverpool Telescope (LT; Steele et al. 2004) on 2019 Oct 23.93 UT. The spectrum shows strong Balmer emission lines (H & alpha;, H & beta;, H & gamma;, H & delta;), along with numerous Fe II emission lines, including those of the 27, 28, 37, 38, 42, 48, 49 and 74 multiplets.
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