D2 Article in a professional compilation book
Spectroscopic Classification of AT 2019pih and M31N 2019-09a as novae in M31
Authors: Williams SC, Darnley MJ, Healy MW, Murphy-Glaysher FJ, Ransome CL
Publication year: 2019
Book title : Astronomer’s telegram
Journal name in source: The Astronomer's Telegram
Series title: Astronomer’s telegram
Number in series: 13078
Web address : https://www.astronomerstelegram.org/?read=13078
Abstract
We obtained a spectrum of the transient AT 2019pih with the SPRAT spectrograph (resolution R 350; Piascik et al. 2014) on the 2-m Liverpool Telescope (LT; Steele et al. 2004) on 2019 Sep 4.08 UT. The spectrum shows narrow Balmer emission lines (H & alpha;, H & beta;, H & gamma;, H & delta;), along with numerous Fe II emission lines, including those of the 37, 38, 42, 48 and 49 multiplets.
We obtained a spectrum of the transient AT 2019pih with the SPRAT spectrograph (resolution R 350; Piascik et al. 2014) on the 2-m Liverpool Telescope (LT; Steele et al. 2004) on 2019 Sep 4.08 UT. The spectrum shows narrow Balmer emission lines (H & alpha;, H & beta;, H & gamma;, H & delta;), along with numerous Fe II emission lines, including those of the 37, 38, 42, 48 and 49 multiplets.
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