A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii

A near-infrared spectrum of nova V1716 Scorpii (PNV J17224490-4137160), a recent bright ( ${V}_{\max }=7.3$ mag), Fermi-LAT detected γ -ray source, was modeled using the photoionization code CLOUDY. Abundances were estimated for He, C, N, O, Si, Al, Mg, Fe, Ne, S, Ca, and P. Notably, P (a factor of...

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Bibliographic Details
Main Authors: C. E. Woodward, G. Shaw, S. Starrfield, A. Evans, K. L. Page
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad4097