VLT VIMOS integral field spectroscopy of the nova remnant FH ser

Context. The source FH Ser experienced a slow classical nova outburst in February 1970 that was the first ever observed at UV, optical, and IR wavelengths. Its nova remnant is elliptical and has multiple knots. A peculiar ring-like filament lies along its minor axis.

Detalhes bibliográficos
Autores: Guerrero, Martín A., Santamaría, E., Takeda, L., González-Carbajal, J. I., Cazzoli, S., Ederoclite, Alessandro, Toalá, Jesús A.
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2025
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/381488
Acesso em linha:http://hdl.handle.net/10261/381488
Access Level:acceso abierto
Palavra-chave:Binaries: general
Novae, cataclysmic variables
ISM: jets and outflows
ISM: individual objects: FH ser
Descrição
Resumo:Context. The source FH Ser experienced a slow classical nova outburst in February 1970 that was the first ever observed at UV, optical, and IR wavelengths. Its nova remnant is elliptical and has multiple knots. A peculiar ring-like filament lies along its minor axis.

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