# High-resolution optical spectroscopy of Nova V392 Per

## TL;DR

This paper presents high-resolution spectral analysis of Nova V392 Per's 2018 outburst, revealing complex emission line structures, rapid decline times, and discussing its classification as a very fast nova and its evolutionary implications.

## Contribution

It provides detailed spectral data and analysis of Nova V392 Per, including emission line profiles, interstellar extinction estimates, and classification as a very fast nova, contributing to understanding nova evolution.

## Key findings

- Triple-peak Hα and Hβ emission lines with high radial velocities
- V392 Per classified as a very fast nova with t₂ ≈ 3 days
- Discussion on the nova's similarity to other very fast novae and future evolution

## Abstract

Here we analyze high-resolution spectra of the Nova V392 Per obtained during the 2018 outburst. The H$\alpha$ and H$\beta$ emission lines show a triple-peak structure with radial velocities of about -2000 km/s, -250 km/s and 1900 km/s respectively. The near infrared spectrum is dominated by the narrow and single-peaked Paschen lines of hydrogen and the OI $\lambda$8446 and OI $\lambda$7773 emission lines. Using DIBs and the KI line, we estimate the interstellar excess towards V392 Per. Based on AAVSO and ASAS-SN photometry data, we calculate that the t$_2$ and t$_3$ decline times are $\sim$ 3 d and $\sim$ 11 d respectively, which classifies V392 Per as a very fast nova. We also briefly discuss the similarity between V392 Per and other very fast novae and the possible future evolution of the system in terms of the hibernation model.