On the evolutionary state of massive stars in transition phases in M33

The advanced stages of several high-mass stars are characterized by episodic mass-loss shed during phases of instability.Key for assigning these stars a proper evolutionary state is to assess the composition and geometry of their ejecta alongside the stellar properties. We selected five hot luminous...

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Autores principales: Kourniotis, M., Kraus, M., Arias, María Laura, Cidale, Lydia Sonia, Torres, Andrea Fabiana
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2018
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/93616
https://academic.oup.com/mnras/article-abstract/480/3/3706/5063594
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id I19-R120-10915-93616
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Infrared: stars
Stars: massive
Stars: winds, outflows
Circumstellar matter
Stars: emission line, Be
Supergiants
spellingShingle Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Infrared: stars
Stars: massive
Stars: winds, outflows
Circumstellar matter
Stars: emission line, Be
Supergiants
Kourniotis, M.
Kraus, M.
Arias, María Laura
Cidale, Lydia Sonia
Torres, Andrea Fabiana
On the evolutionary state of massive stars in transition phases in M33
topic_facet Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Infrared: stars
Stars: massive
Stars: winds, outflows
Circumstellar matter
Stars: emission line, Be
Supergiants
description The advanced stages of several high-mass stars are characterized by episodic mass-loss shed during phases of instability.Key for assigning these stars a proper evolutionary state is to assess the composition and geometry of their ejecta alongside the stellar properties. We selected five hot luminous blue variable candidates in M33 to refine their classification, investigate their circumstellar environments, and explore their evolutionary properties. Being accessible targets in the near-infrared, we conducted medium-resolution spectroscopy with GNIRS/GEMINI in the K-band to investigate their molecular circumstellar environments. Two stars were found to display CO emission, which was modelled to emerge from a circumstellar or circumbinary Keplerian disc/ring. The identification of the carbon isotope 13C and, for one of the two stars, a significantly low 12CO/13CO ratio, implies an evolved stellar state. As both CO emission stars are highly luminous and hence do not undergo a red supergiant phase, we suggest that stripping processes and equatorial high-density ejecta due to fast rotation are responsible for the enrichment of the stellar surface with processedmaterial from the core.Acandidate B[e]SG displays an absorption CO profile, which may be attributed to a jet or stellar pulsations. The featureless infrared spectra of two stars suggest a low-density gas shell or dissipation of the molecule due to the ionizing temperature of the star. We propose spectroscopic monitoring of our targets to evaluate the stability of the CO molecule and assess the time-dependent dynamics of the circumstellar gas structures.
format Articulo
Preprint
author Kourniotis, M.
Kraus, M.
Arias, María Laura
Cidale, Lydia Sonia
Torres, Andrea Fabiana
author_facet Kourniotis, M.
Kraus, M.
Arias, María Laura
Cidale, Lydia Sonia
Torres, Andrea Fabiana
author_sort Kourniotis, M.
title On the evolutionary state of massive stars in transition phases in M33
title_short On the evolutionary state of massive stars in transition phases in M33
title_full On the evolutionary state of massive stars in transition phases in M33
title_fullStr On the evolutionary state of massive stars in transition phases in M33
title_full_unstemmed On the evolutionary state of massive stars in transition phases in M33
title_sort on the evolutionary state of massive stars in transition phases in m33
publishDate 2018
url http://sedici.unlp.edu.ar/handle/10915/93616
https://academic.oup.com/mnras/article-abstract/480/3/3706/5063594
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