Chemistry and physical properties of the born-Again planetary nebula HuBi 1
- Autores
- Montoro Molina, B; Guerrero, M. A.; Perez Díaz, B.; Toalá, J. A.; Cazzoli, S.; Miller Bertolami, Marcelo Miguel; Morisset, C.
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The central star of the planetary nebula (PN) HuBi 1 has been recently proposed to have experienced a very late thermal pulse (VLTP), but the dilution of the emission of the recent ejecta by that of the surrounding H-rich old outer shell has so far hindered confirming its suspected H-poor nature. We present here an analysis of the optical properties of the ejecta in the innermost regions of HuBi 1 using MEGARA high-dispersion integral field and OSIRIS intermediate-dispersion long-slit spectroscopic observations obtained with the 10.4-m Gran Telescopio de Canarias. The unprecedented tomographic capability of MEGARA to resolve structures in velocity space allowed us to disentangle for the first time the Hα and Hβ emission of the recent ejecta from that of the outer shell. The recent ejecta is found to have much higher extinction than the outer shell, implying the presence of large amounts of dust. The spatial distribution of the emission from the ejecta and the locus of key line ratios in diagnostic diagrams probe the shock excitation of the inner ejecta in HuBi 1, in stark contrast with the photoionization nature of the H-rich outer shell. The abundances of the recent ejecta have been computed using the mappings v code under a shock scenario. They are found to be consistent with a born-Again ejection scenario experienced by the progenitor star, which is thus firmly confirmed as a new 'born-Again' star.
Fil: Montoro Molina, B. Consejo Superior de Investigaciones Científicas; España
Fil: Guerrero, M. A.. Consejo Superior de Investigaciones Científicas; España
Fil: Perez Díaz, B.. Consejo Superior de Investigaciones Científicas; España
Fil: Toalá, J. A.. Universidad Nacional Autónoma de México; México
Fil: Cazzoli, S.. Consejo Superior de Investigaciones Científicas; España
Fil: Miller Bertolami, Marcelo Miguel. 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: Morisset, C.. Universidad Nacional Autónoma de México; México - Materia
-
ISM: JETS AND OUTFLOWS
PLANETARY NEBULAE: GENERAL
PLANETARY NEBULAE: INDIVIDUAL (HUBI 1)
STARS: EVOLUTION
STARS: WINDS, OUTFLOWS - 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:11336/210870
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network_name_str |
CONICET Digital (CONICET) |
spelling |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1Montoro Molina, BGuerrero, M. A.Perez Díaz, B.Toalá, J. A.Cazzoli, S.Miller Bertolami, Marcelo MiguelMorisset, C.ISM: JETS AND OUTFLOWSPLANETARY NEBULAE: GENERALPLANETARY NEBULAE: INDIVIDUAL (HUBI 1)STARS: EVOLUTIONSTARS: WINDS, OUTFLOWShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The central star of the planetary nebula (PN) HuBi 1 has been recently proposed to have experienced a very late thermal pulse (VLTP), but the dilution of the emission of the recent ejecta by that of the surrounding H-rich old outer shell has so far hindered confirming its suspected H-poor nature. We present here an analysis of the optical properties of the ejecta in the innermost regions of HuBi 1 using MEGARA high-dispersion integral field and OSIRIS intermediate-dispersion long-slit spectroscopic observations obtained with the 10.4-m Gran Telescopio de Canarias. The unprecedented tomographic capability of MEGARA to resolve structures in velocity space allowed us to disentangle for the first time the Hα and Hβ emission of the recent ejecta from that of the outer shell. The recent ejecta is found to have much higher extinction than the outer shell, implying the presence of large amounts of dust. The spatial distribution of the emission from the ejecta and the locus of key line ratios in diagnostic diagrams probe the shock excitation of the inner ejecta in HuBi 1, in stark contrast with the photoionization nature of the H-rich outer shell. The abundances of the recent ejecta have been computed using the mappings v code under a shock scenario. They are found to be consistent with a born-Again ejection scenario experienced by the progenitor star, which is thus firmly confirmed as a new 'born-Again' star.Fil: Montoro Molina, B. Consejo Superior de Investigaciones Científicas; EspañaFil: Guerrero, M. A.. Consejo Superior de Investigaciones Científicas; EspañaFil: Perez Díaz, B.. Consejo Superior de Investigaciones Científicas; EspañaFil: Toalá, J. A.. Universidad Nacional Autónoma de México; MéxicoFil: Cazzoli, S.. Consejo Superior de Investigaciones Científicas; EspañaFil: Miller Bertolami, Marcelo Miguel. 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: Morisset, C.. Universidad Nacional Autónoma de México; MéxicoWiley Blackwell Publishing, Inc2022-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/210870Montoro Molina, B; Guerrero, M. A.; Perez Díaz, B.; Toalá, J. A.; Cazzoli, S.; et al.; Chemistry and physical properties of the born-Again planetary nebula HuBi 1; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 512; 3; 5-2022; 4003-40200035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/512/3/4003/6527589info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac336info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:03:35Zoai:ri.conicet.gov.ar:11336/210870instacron: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:34982025-09-29 10:03:35.558CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1 |
title |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1 |
spellingShingle |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1 Montoro Molina, B ISM: JETS AND OUTFLOWS PLANETARY NEBULAE: GENERAL PLANETARY NEBULAE: INDIVIDUAL (HUBI 1) STARS: EVOLUTION STARS: WINDS, OUTFLOWS |
title_short |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1 |
title_full |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1 |
title_fullStr |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1 |
title_full_unstemmed |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1 |
title_sort |
Chemistry and physical properties of the born-Again planetary nebula HuBi 1 |
dc.creator.none.fl_str_mv |
Montoro Molina, B Guerrero, M. A. Perez Díaz, B. Toalá, J. A. Cazzoli, S. Miller Bertolami, Marcelo Miguel Morisset, C. |
author |
Montoro Molina, B |
author_facet |
Montoro Molina, B Guerrero, M. A. Perez Díaz, B. Toalá, J. A. Cazzoli, S. Miller Bertolami, Marcelo Miguel Morisset, C. |
author_role |
author |
author2 |
Guerrero, M. A. Perez Díaz, B. Toalá, J. A. Cazzoli, S. Miller Bertolami, Marcelo Miguel Morisset, C. |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
ISM: JETS AND OUTFLOWS PLANETARY NEBULAE: GENERAL PLANETARY NEBULAE: INDIVIDUAL (HUBI 1) STARS: EVOLUTION STARS: WINDS, OUTFLOWS |
topic |
ISM: JETS AND OUTFLOWS PLANETARY NEBULAE: GENERAL PLANETARY NEBULAE: INDIVIDUAL (HUBI 1) STARS: EVOLUTION STARS: WINDS, OUTFLOWS |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The central star of the planetary nebula (PN) HuBi 1 has been recently proposed to have experienced a very late thermal pulse (VLTP), but the dilution of the emission of the recent ejecta by that of the surrounding H-rich old outer shell has so far hindered confirming its suspected H-poor nature. We present here an analysis of the optical properties of the ejecta in the innermost regions of HuBi 1 using MEGARA high-dispersion integral field and OSIRIS intermediate-dispersion long-slit spectroscopic observations obtained with the 10.4-m Gran Telescopio de Canarias. The unprecedented tomographic capability of MEGARA to resolve structures in velocity space allowed us to disentangle for the first time the Hα and Hβ emission of the recent ejecta from that of the outer shell. The recent ejecta is found to have much higher extinction than the outer shell, implying the presence of large amounts of dust. The spatial distribution of the emission from the ejecta and the locus of key line ratios in diagnostic diagrams probe the shock excitation of the inner ejecta in HuBi 1, in stark contrast with the photoionization nature of the H-rich outer shell. The abundances of the recent ejecta have been computed using the mappings v code under a shock scenario. They are found to be consistent with a born-Again ejection scenario experienced by the progenitor star, which is thus firmly confirmed as a new 'born-Again' star. Fil: Montoro Molina, B. Consejo Superior de Investigaciones Científicas; España Fil: Guerrero, M. A.. Consejo Superior de Investigaciones Científicas; España Fil: Perez Díaz, B.. Consejo Superior de Investigaciones Científicas; España Fil: Toalá, J. A.. Universidad Nacional Autónoma de México; México Fil: Cazzoli, S.. Consejo Superior de Investigaciones Científicas; España Fil: Miller Bertolami, Marcelo Miguel. 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: Morisset, C.. Universidad Nacional Autónoma de México; México |
description |
The central star of the planetary nebula (PN) HuBi 1 has been recently proposed to have experienced a very late thermal pulse (VLTP), but the dilution of the emission of the recent ejecta by that of the surrounding H-rich old outer shell has so far hindered confirming its suspected H-poor nature. We present here an analysis of the optical properties of the ejecta in the innermost regions of HuBi 1 using MEGARA high-dispersion integral field and OSIRIS intermediate-dispersion long-slit spectroscopic observations obtained with the 10.4-m Gran Telescopio de Canarias. The unprecedented tomographic capability of MEGARA to resolve structures in velocity space allowed us to disentangle for the first time the Hα and Hβ emission of the recent ejecta from that of the outer shell. The recent ejecta is found to have much higher extinction than the outer shell, implying the presence of large amounts of dust. The spatial distribution of the emission from the ejecta and the locus of key line ratios in diagnostic diagrams probe the shock excitation of the inner ejecta in HuBi 1, in stark contrast with the photoionization nature of the H-rich outer shell. The abundances of the recent ejecta have been computed using the mappings v code under a shock scenario. They are found to be consistent with a born-Again ejection scenario experienced by the progenitor star, which is thus firmly confirmed as a new 'born-Again' star. |
publishDate |
2022 |
dc.date.none.fl_str_mv |
2022-05 |
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/11336/210870 Montoro Molina, B; Guerrero, M. A.; Perez Díaz, B.; Toalá, J. A.; Cazzoli, S.; et al.; Chemistry and physical properties of the born-Again planetary nebula HuBi 1; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 512; 3; 5-2022; 4003-4020 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/210870 |
identifier_str_mv |
Montoro Molina, B; Guerrero, M. A.; Perez Díaz, B.; Toalá, J. A.; Cazzoli, S.; et al.; Chemistry and physical properties of the born-Again planetary nebula HuBi 1; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 512; 3; 5-2022; 4003-4020 0035-8711 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/512/3/4003/6527589 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac336 |
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/pdf |
dc.publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
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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1844613854007394304 |
score |
13.070432 |