Robiatul Muztaba, Hakim L. Malasan, Akira Arai
Novae V5668 Sgr spectra that have been observed at Bosscha Observatory on June 12, June 23 and August 15, 2015 using the NEO-R1000 spectrograph attached to the C-11 telescope showed that it has been entered the nebular phase. We will present the results of photoionization modelling using CLOUDY from observations of the Novae V5668 Sgr. The results of this modelling show that the spectrum profile matches fairly to the observations. Emission line features such as H, [O I] λ 6300, 6364 Å, [O II] λ 7320 Å, [O III] λ 5007 Å, [N II] λ 5755 Å, and Fe II λ 4924, 5169, 5317, 6149 Å on the observed spectra are also well formed and represented by the model. © 2020 Published under licence by IOP Publishing Ltd.
Department of Atmospheric and Planetary Sciences, Institut Teknologi Sumatera, Lampung, 35365, Indonesia; Astronomy Division and Bosscha Observatory, Institut Teknologi Bandung, Bandung, 40132, Indonesia; Itera Astronomical Observatory, Institut Teknologi Sumatera, Lampung, 35365, Indonesia; Koyama Astronomical Observatory, Kyoto Sangyo University, Motoyama, Kamigamo, Kitaku, Kyoto, 603-8555, Japan
Research at a Glance
Register to unlock
Topics & SDG Alignment
Register to unlock
Collaboration
Register to unlock
Author Profile (Selected)
Register to unlock
References Overview
Register to unlock
Journal & Source
Register to unlock
Metadata & Integrity
Register to unlock