CCD images and long-slit spectroscopy of the ring nebula around θ Mus

We present the first digital CCD images and long-slit spectroscopy of the optical ring nebula around the Wolf-Rayet star θ Mus. The CCD images obtained through narrow-band filters centred at [O III] and Hα show that the nebula has a filamentary structure, similar to supernova remnants, mainly seen i...

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Autores principales: De Castro, C.G.G., Niemela, V.S.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00358711_v297_n4_p1060_DeCastro
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spelling todo:paper_00358711_v297_n4_p1060_DeCastro2023-10-03T14:46:39Z CCD images and long-slit spectroscopy of the ring nebula around θ Mus De Castro, C.G.G. Niemela, V.S. ISM: bubbles Stars: individual: HD 113904 Stars: Wolf-Rayet We present the first digital CCD images and long-slit spectroscopy of the optical ring nebula around the Wolf-Rayet star θ Mus. The CCD images obtained through narrow-band filters centred at [O III] and Hα show that the nebula has a filamentary structure, similar to supernova remnants, mainly seen in [O III]. A spatial detachment between [O III] and Ha images suggests excitation stratification, or multiple rings. An analysis of the physical conditions in the nebula was performed by means of long-slit CCD spectra. The spectral images show that the nebula is of low density and medium excitation. By means of quotients of recombination and collisional spectral line fluxes we determine that the principal excitation mechanism is photoionization. We have determined the electronic temperature and density, and chemical abundances for the oxygen at different sites within the nebula. Nebular chemical abundances are found to be similar to the Galactic ISM, indicating that the nebula is mainly composed of swept up material. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00358711_v297_n4_p1060_DeCastro
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic ISM: bubbles
Stars: individual: HD 113904
Stars: Wolf-Rayet
spellingShingle ISM: bubbles
Stars: individual: HD 113904
Stars: Wolf-Rayet
De Castro, C.G.G.
Niemela, V.S.
CCD images and long-slit spectroscopy of the ring nebula around θ Mus
topic_facet ISM: bubbles
Stars: individual: HD 113904
Stars: Wolf-Rayet
description We present the first digital CCD images and long-slit spectroscopy of the optical ring nebula around the Wolf-Rayet star θ Mus. The CCD images obtained through narrow-band filters centred at [O III] and Hα show that the nebula has a filamentary structure, similar to supernova remnants, mainly seen in [O III]. A spatial detachment between [O III] and Ha images suggests excitation stratification, or multiple rings. An analysis of the physical conditions in the nebula was performed by means of long-slit CCD spectra. The spectral images show that the nebula is of low density and medium excitation. By means of quotients of recombination and collisional spectral line fluxes we determine that the principal excitation mechanism is photoionization. We have determined the electronic temperature and density, and chemical abundances for the oxygen at different sites within the nebula. Nebular chemical abundances are found to be similar to the Galactic ISM, indicating that the nebula is mainly composed of swept up material.
format JOUR
author De Castro, C.G.G.
Niemela, V.S.
author_facet De Castro, C.G.G.
Niemela, V.S.
author_sort De Castro, C.G.G.
title CCD images and long-slit spectroscopy of the ring nebula around θ Mus
title_short CCD images and long-slit spectroscopy of the ring nebula around θ Mus
title_full CCD images and long-slit spectroscopy of the ring nebula around θ Mus
title_fullStr CCD images and long-slit spectroscopy of the ring nebula around θ Mus
title_full_unstemmed CCD images and long-slit spectroscopy of the ring nebula around θ Mus
title_sort ccd images and long-slit spectroscopy of the ring nebula around θ mus
url http://hdl.handle.net/20.500.12110/paper_00358711_v297_n4_p1060_DeCastro
work_keys_str_mv AT decastrocgg ccdimagesandlongslitspectroscopyoftheringnebulaaroundthmus
AT niemelavs ccdimagesandlongslitspectroscopyoftheringnebulaaroundthmus
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