V1369 Cen High-resolution Panchromatic Late Nebular Spectra in the Context of a Unified Picture for Nova Ejecta

• Published in: The Astrophysical Journal
• Main Authors: Mason, E, Shore, SN, Aquino, IDG, Izzo, L, Page, K, Schwarz, GJ
• Format: Article in Journal/Newspaper
• Language: English
• Published: American Astronomical Society, IOP Publishing 2019
• Subjects: Science & Technology; Physical Sciences; Astronomy & Astrophysics; stars: novae; cataclysmic variables; stars: individual (V339 Del; V1369 Cen; V959 Mon); line: formation; line: identification; line: profiles; methods: observational; techniques: spectroscopic; GROUND-BASED SPECTROSCOPY; CLASSICAL NOVAE; ABSORPTION SYSTEMS; MASS EJECTION; ULTRAVIOLET; EMISSION; CYG; EVOLUTION; SHELLS; RADIO; Norway; Osborne; Hubble; Observatorio; Sumner; Iceland
• Online Access: https://iopscience.iop.org/article/10.3847/1538-4357/aaa247; http://hdl.handle.net/2381/44707; https://doi.org/10.3847/1538-4357/aaa247

Nova Cen 2013 (V1369 Cen) is the fourth bright nova observed panchromatically through high-resolution UV +optical multiepoch spectroscopy. It is also the nova with the richest set of spectra (in terms of both data quality and number of epochs) thanks to its exceptional brightness. Here, we use the l...