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
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/210870
Acceder
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network_acronym_str CONICETDig
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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 Técnicas2025-10-22T11:33:22Zoai: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:34982025-10-22 11:33:22.709CONICET 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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score 12.982451

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