Ring nebulae around Wolf-Rayet stars in M33 as seen by SITELLE

Fuente: arXiv
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Autores principales: Tuquet, Selin, -Louis, Nicole St., Drissen, Laurent, Raaijmakers, Sylvain, Rousseau-Nepton, Laurie, Martin, René Pierre, Robert, Carmelle, Amram, Philippe
Formato: Preprint
Publicado: 2024
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author Tuquet, Selin
-Louis, Nicole St.
Drissen, Laurent
Raaijmakers, Sylvain
Rousseau-Nepton, Laurie
Martin, René Pierre
Robert, Carmelle
Amram, Philippe
author_facet Tuquet, Selin
-Louis, Nicole St.
Drissen, Laurent
Raaijmakers, Sylvain
Rousseau-Nepton, Laurie
Martin, René Pierre
Robert, Carmelle
Amram, Philippe
contents We have conducted an analysis of nebulae around Wolf-Rayet (WR) stars in M33 using data collected by the imaging Fourier transform spectrometer SITELLE at the Canada-France-Hawaii telescope as part of the SIGNALS Large Program. Of the 211 known Wolf-Rayet stars in M33, 178 are located in the fields observed in this study. We present the results of this analysis in the form of a comprehensive summary of all nebulae found around the observed WR stars. Based on three criteria we find to be the most effective for their detection, we detect a clear association with a circumstellar bubble around 33 of them (19\%). Our results show that the presence of bubbles does not correlate with the spectral type of the central star. The mean diameter of the WR nebulae we have found is 21 parsecs.
format Preprint
id arxiv_https___arxiv_org_abs_2403_12754
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Ring nebulae around Wolf-Rayet stars in M33 as seen by SITELLE
Tuquet, Selin
-Louis, Nicole St.
Drissen, Laurent
Raaijmakers, Sylvain
Rousseau-Nepton, Laurie
Martin, René Pierre
Robert, Carmelle
Amram, Philippe
Solar and Stellar Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
We have conducted an analysis of nebulae around Wolf-Rayet (WR) stars in M33 using data collected by the imaging Fourier transform spectrometer SITELLE at the Canada-France-Hawaii telescope as part of the SIGNALS Large Program. Of the 211 known Wolf-Rayet stars in M33, 178 are located in the fields observed in this study. We present the results of this analysis in the form of a comprehensive summary of all nebulae found around the observed WR stars. Based on three criteria we find to be the most effective for their detection, we detect a clear association with a circumstellar bubble around 33 of them (19\%). Our results show that the presence of bubbles does not correlate with the spectral type of the central star. The mean diameter of the WR nebulae we have found is 21 parsecs.
title Ring nebulae around Wolf-Rayet stars in M33 as seen by SITELLE
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2403.12754