VLT VIMOS Integral Field Spectroscopy of the nova remnant FH Ser
M.A. Guerrero, E. Santamaria, L. Takeda, J.I. Gonzalez-Carbajal, S., Cazzoli, A. Ederoclite, J.A. Toala

TL;DR
This study uses VLT VIMOS integral field spectroscopy to analyze the 3D structure of the FH Ser nova remnant, revealing a tilted ellipsoidal shell and ring-like structure, and estimating its mass and energy.
Contribution
It provides the first detailed 3D kinematic model of FH Ser's nova remnant using integral field spectroscopy, highlighting structural components and their orientations.
Findings
FH Ser has a tilted prolate ellipsoidal shell with specific velocities.
A ring-like structure is identified, aligned with the shell.
Ionized mass and kinetic energy of the remnant are quantified.
Abstract
FH Ser experienced a slow classical nova outburst in February 1970 that was the first one observed at UV, optical, and IR wavelengths. Its nova remnant is elliptical in shape, with multiple knots, and a peculiar ring-like filament along its minor axis. This work aims at unveiling its true 3D spatio-kinematical structure to investigate the effects of early shaping and to assess its mass and kinetic energy using VLT VIMOS integral field spectroscopic observations. The data cube has been analyzed using 3D visualisations that reveal different structural components. FH Ser consists of a tilted prolate ellisoidal shell, most prominent in H-alpha, and a ring-like structure, most prominent in [N II]. The ellipsoidal shell has equatorial and polar velocities of 505 and 630 km/s, respectively, with its major axis tilted by 52 deg with respect to the line of sight. The inclination angle of the…
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