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Auteurs principaux: Van de Steene, Griet, van Hoof, Peter, Kimeswenger, Stefan, Hajduk, Marcin, Tafoya, Daniel, Toala, Jesus, Zijlstra, Albert, Barria, Daniela
Format: Preprint
Publié: 2024
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Accès en ligne:https://arxiv.org/abs/2409.13289
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author Van de Steene, Griet
van Hoof, Peter
Kimeswenger, Stefan
Hajduk, Marcin
Tafoya, Daniel
Toala, Jesus
Zijlstra, Albert
Barria, Daniela
author_facet Van de Steene, Griet
van Hoof, Peter
Kimeswenger, Stefan
Hajduk, Marcin
Tafoya, Daniel
Toala, Jesus
Zijlstra, Albert
Barria, Daniela
contents Optical spectra of the Very Late Thermal Pulse (VLTP) object V4334 Sgr have shown a rapidly changing spectrum resulting from shocks in the outflow, which created a new bipolar nebula inside the old nebula. We see C II and C III emission lines emerging typical of a [WC 11-10]-type star. The strong increase of [O III] and [S III] emission lines indicate the possible onset of photoionisation in the new ejecta.
format Preprint
id arxiv_https___arxiv_org_abs_2409_13289
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Sakurai's object: a [WC] star in a new bipolar nebula after a VLTP
Van de Steene, Griet
van Hoof, Peter
Kimeswenger, Stefan
Hajduk, Marcin
Tafoya, Daniel
Toala, Jesus
Zijlstra, Albert
Barria, Daniela
Solar and Stellar Astrophysics
Astrophysics of Galaxies
High Energy Astrophysical Phenomena
Optical spectra of the Very Late Thermal Pulse (VLTP) object V4334 Sgr have shown a rapidly changing spectrum resulting from shocks in the outflow, which created a new bipolar nebula inside the old nebula. We see C II and C III emission lines emerging typical of a [WC 11-10]-type star. The strong increase of [O III] and [S III] emission lines indicate the possible onset of photoionisation in the new ejecta.
title Sakurai's object: a [WC] star in a new bipolar nebula after a VLTP
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2409.13289