Unveiling the Environments of Extreme Massive Stars
- Autores
- Kraus, M.; Liimets, Tiina; Arias, María Laura; Moiseev, A.; Cidale, Lydia Sonia; Torres, Andrea Fabiana; Nickeler , Dieter H.
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Massive stars are powerful cosmic engines, enriching their environments withenergy and mass throughout their lifetime. The post-main sequence evolutionof massive stars comprises several distinct states, such as the luminous bluevariables, blue supergiants, red supergiants, Wolf-Rayet stars, B[e] supergiantsand yellow hypergiants, many of them connected with intense mass loss,embedding the stars in a dense environment. Here we present an overviewof our studies for members in three states of evolved massive stars: B[e]supergiants, luminous blue variables, and yellow hypergiants. Combininghigh-quality spectral and imaging observations over large wavelength regions,we aim to unveil the physical properties and temporal evolution of theejected material in these types of objects in order to gain insight into theirmass loss and mass ejection histories. This information is also vital to constrain the location of these objects along the evolutionary path of massive stars.
Fil: Kraus, M.. Czech Academy of Sciences; República Checa
Fil: Liimets, Tiina. Czech Academy of Sciences; República Checa
Fil: Arias, María Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Moiseev, A.. Academia de Ciencias de Rusia.; Rusia
Fil: Cidale, Lydia Sonia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Torres, Andrea Fabiana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Nickeler , Dieter H.. Czech Academy of Sciences; República Checa - Materia
-
stars: massive
supergiants
circumstellar matters - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/247032
Ver los metadatos del registro completo
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Unveiling the Environments of Extreme Massive StarsKraus, M.Liimets, TiinaArias, María LauraMoiseev, A.Cidale, Lydia SoniaTorres, Andrea FabianaNickeler , Dieter H.stars: massivesupergiantscircumstellar mattershttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Massive stars are powerful cosmic engines, enriching their environments withenergy and mass throughout their lifetime. The post-main sequence evolutionof massive stars comprises several distinct states, such as the luminous bluevariables, blue supergiants, red supergiants, Wolf-Rayet stars, B[e] supergiantsand yellow hypergiants, many of them connected with intense mass loss,embedding the stars in a dense environment. Here we present an overviewof our studies for members in three states of evolved massive stars: B[e]supergiants, luminous blue variables, and yellow hypergiants. Combininghigh-quality spectral and imaging observations over large wavelength regions,we aim to unveil the physical properties and temporal evolution of theejected material in these types of objects in order to gain insight into theirmass loss and mass ejection histories. This information is also vital to constrain the location of these objects along the evolutionary path of massive stars.Fil: Kraus, M.. Czech Academy of Sciences; República ChecaFil: Liimets, Tiina. Czech Academy of Sciences; República ChecaFil: Arias, María Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Moiseev, A.. Academia de Ciencias de Rusia.; RusiaFil: Cidale, Lydia Sonia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Torres, Andrea Fabiana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Nickeler , Dieter H.. Czech Academy of Sciences; República ChecaAzerbaijan National Academy of Sciences2022-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/zipapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/247032Kraus, M.; Liimets, Tiina; Arias, María Laura; Moiseev, A.; Cidale, Lydia Sonia; et al.; Unveiling the Environments of Extreme Massive Stars; Azerbaijan National Academy of Sciences; Azerbaijani Astronomical Journal; 17; 2; 12-2022; 7-222078-4171CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://aaj.shao.az/vol17_n2/AAJ_2022_V17_N2.pdfinfo:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2022AzAJ...17b...7K/abstractinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:50:16Zoai:ri.conicet.gov.ar:11336/247032instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:50:17.312CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Unveiling the Environments of Extreme Massive Stars |
title |
Unveiling the Environments of Extreme Massive Stars |
spellingShingle |
Unveiling the Environments of Extreme Massive Stars Kraus, M. stars: massive supergiants circumstellar matters |
title_short |
Unveiling the Environments of Extreme Massive Stars |
title_full |
Unveiling the Environments of Extreme Massive Stars |
title_fullStr |
Unveiling the Environments of Extreme Massive Stars |
title_full_unstemmed |
Unveiling the Environments of Extreme Massive Stars |
title_sort |
Unveiling the Environments of Extreme Massive Stars |
dc.creator.none.fl_str_mv |
Kraus, M. Liimets, Tiina Arias, María Laura Moiseev, A. Cidale, Lydia Sonia Torres, Andrea Fabiana Nickeler , Dieter H. |
author |
Kraus, M. |
author_facet |
Kraus, M. Liimets, Tiina Arias, María Laura Moiseev, A. Cidale, Lydia Sonia Torres, Andrea Fabiana Nickeler , Dieter H. |
author_role |
author |
author2 |
Liimets, Tiina Arias, María Laura Moiseev, A. Cidale, Lydia Sonia Torres, Andrea Fabiana Nickeler , Dieter H. |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
stars: massive supergiants circumstellar matters |
topic |
stars: massive supergiants circumstellar matters |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Massive stars are powerful cosmic engines, enriching their environments withenergy and mass throughout their lifetime. The post-main sequence evolutionof massive stars comprises several distinct states, such as the luminous bluevariables, blue supergiants, red supergiants, Wolf-Rayet stars, B[e] supergiantsand yellow hypergiants, many of them connected with intense mass loss,embedding the stars in a dense environment. Here we present an overviewof our studies for members in three states of evolved massive stars: B[e]supergiants, luminous blue variables, and yellow hypergiants. Combininghigh-quality spectral and imaging observations over large wavelength regions,we aim to unveil the physical properties and temporal evolution of theejected material in these types of objects in order to gain insight into theirmass loss and mass ejection histories. This information is also vital to constrain the location of these objects along the evolutionary path of massive stars. Fil: Kraus, M.. Czech Academy of Sciences; República Checa Fil: Liimets, Tiina. Czech Academy of Sciences; República Checa Fil: Arias, María Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Moiseev, A.. Academia de Ciencias de Rusia.; Rusia Fil: Cidale, Lydia Sonia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Torres, Andrea Fabiana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Nickeler , Dieter H.. Czech Academy of Sciences; República Checa |
description |
Massive stars are powerful cosmic engines, enriching their environments withenergy and mass throughout their lifetime. The post-main sequence evolutionof massive stars comprises several distinct states, such as the luminous bluevariables, blue supergiants, red supergiants, Wolf-Rayet stars, B[e] supergiantsand yellow hypergiants, many of them connected with intense mass loss,embedding the stars in a dense environment. Here we present an overviewof our studies for members in three states of evolved massive stars: B[e]supergiants, luminous blue variables, and yellow hypergiants. Combininghigh-quality spectral and imaging observations over large wavelength regions,we aim to unveil the physical properties and temporal evolution of theejected material in these types of objects in order to gain insight into theirmass loss and mass ejection histories. This information is also vital to constrain the location of these objects along the evolutionary path of massive stars. |
publishDate |
2022 |
dc.date.none.fl_str_mv |
2022-12 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/247032 Kraus, M.; Liimets, Tiina; Arias, María Laura; Moiseev, A.; Cidale, Lydia Sonia; et al.; Unveiling the Environments of Extreme Massive Stars; Azerbaijan National Academy of Sciences; Azerbaijani Astronomical Journal; 17; 2; 12-2022; 7-22 2078-4171 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/247032 |
identifier_str_mv |
Kraus, M.; Liimets, Tiina; Arias, María Laura; Moiseev, A.; Cidale, Lydia Sonia; et al.; Unveiling the Environments of Extreme Massive Stars; Azerbaijan National Academy of Sciences; Azerbaijani Astronomical Journal; 17; 2; 12-2022; 7-22 2078-4171 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://aaj.shao.az/vol17_n2/AAJ_2022_V17_N2.pdf info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2022AzAJ...17b...7K/abstract |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/zip application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Azerbaijan National Academy of Sciences |
publisher.none.fl_str_mv |
Azerbaijan National Academy of Sciences |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1842269021354852352 |
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13.13397 |