NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?

Autores
Miller Bertolami, Marcelo Miguel; Rohrmann, R. D.; Granada, A.; Althaus, Leandro Gabriel
Año de publicación
2011
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We argue that NSV 11749, an eWe argue that NSV 11749, an eruption observed in the early twentieth century, was a rare event known as “very late thermal pulse” (VLTP). To support our argument we compare the light curve of NSV 11749 with those of the two bona fide VLTP objects known to date, V4334 Sgr and V605 Aql, and with those predicted by state-of-the-art stellar evolution models. Next, we explore the INT Photometric H-Alpha Survey (IPHAS) and Two Micron All Sky Survey (2MASS) catalogs for possible counterparts of the eruption. Our analysis shows that the VLTP scenario outperforms all other proposed scenarios as an explanation of NSV 11749. We identify an IPHAS/2MASS source at the eruption location of NSV 11749. The derived colors suggest that the object is not enshrouded in a thick dust shell as V605 Aql and V4334 Sgr. Also, the absence of an apparent planetary nebula at the eruption location suggests differences with known VLTP objects which might be linked to the intensity of the eruption and the mass of the object. Further exploration of this source and scenario seems desirable. If NSV 11749 was a born-again star, it would be the third event of its kind to have been observed and will strongly help us to increase our understanding of the later stages of stellar evolution and violent reactive convective burning.
Fil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Rohrmann, R. D.. Consejo Nacional de Investigaciones Cientiâ­ficas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina
Fil: Granada, A.. Observatoire Astronomique de l’Universite de Genéeve; Suiza
Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Materia
Cataclysmic Variables ­
Agb And Post-Agb ­
Nsv 11749 (Estrella)
V4334 Sgr (Estrella)
V605 Aql (Estrella)
Novae
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:11336/10084

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network_name_str CONICET Digital (CONICET)
spelling NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?Miller Bertolami, Marcelo MiguelRohrmann, R. D.Granada, A.Althaus, Leandro GabrielCataclysmic Variables ­Agb And Post-Agb ­Nsv 11749 (Estrella)V4334 Sgr (Estrella)V605 Aql (Estrella)Novaehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We argue that NSV 11749, an eWe argue that NSV 11749, an eruption observed in the early twentieth century, was a rare event known as “very late thermal pulse” (VLTP). To support our argument we compare the light curve of NSV 11749 with those of the two bona fide VLTP objects known to date, V4334 Sgr and V605 Aql, and with those predicted by state-of-the-art stellar evolution models. Next, we explore the INT Photometric H-Alpha Survey (IPHAS) and Two Micron All Sky Survey (2MASS) catalogs for possible counterparts of the eruption. Our analysis shows that the VLTP scenario outperforms all other proposed scenarios as an explanation of NSV 11749. We identify an IPHAS/2MASS source at the eruption location of NSV 11749. The derived colors suggest that the object is not enshrouded in a thick dust shell as V605 Aql and V4334 Sgr. Also, the absence of an apparent planetary nebula at the eruption location suggests differences with known VLTP objects which might be linked to the intensity of the eruption and the mass of the object. Further exploration of this source and scenario seems desirable. If NSV 11749 was a born-again star, it would be the third event of its kind to have been observed and will strongly help us to increase our understanding of the later stages of stellar evolution and violent reactive convective burning.Fil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Rohrmann, R. D.. Consejo Nacional de Investigaciones Cientiâ­ficas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; ArgentinaFil: Granada, A.. Observatoire Astronomique de l’Universite de Genéeve; SuizaFil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaIop Publishing2011-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/10084Miller Bertolami, Marcelo Miguel; Rohrmann, R. D.; Granada, A.; Althaus, Leandro Gabriel; NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?; Iop Publishing; Astrophysical Journal; 743; 2; 12-2011; 1-60004-637Xenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/743/2/L33/metainfo:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/743/2/L33info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:41:24Zoai:ri.conicet.gov.ar:11336/10084instacron: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 11:41:25.044CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?
title NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?
spellingShingle NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?
Miller Bertolami, Marcelo Miguel
Cataclysmic Variables ­
Agb And Post-Agb ­
Nsv 11749 (Estrella)
V4334 Sgr (Estrella)
V605 Aql (Estrella)
Novae
title_short NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?
title_full NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?
title_fullStr NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?
title_full_unstemmed NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?
title_sort NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?
dc.creator.none.fl_str_mv Miller Bertolami, Marcelo Miguel
Rohrmann, R. D.
Granada, A.
Althaus, Leandro Gabriel
author Miller Bertolami, Marcelo Miguel
author_facet Miller Bertolami, Marcelo Miguel
Rohrmann, R. D.
Granada, A.
Althaus, Leandro Gabriel
author_role author
author2 Rohrmann, R. D.
Granada, A.
Althaus, Leandro Gabriel
author2_role author
author
author
dc.subject.none.fl_str_mv Cataclysmic Variables ­
Agb And Post-Agb ­
Nsv 11749 (Estrella)
V4334 Sgr (Estrella)
V605 Aql (Estrella)
Novae
topic Cataclysmic Variables ­
Agb And Post-Agb ­
Nsv 11749 (Estrella)
V4334 Sgr (Estrella)
V605 Aql (Estrella)
Novae
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We argue that NSV 11749, an eWe argue that NSV 11749, an eruption observed in the early twentieth century, was a rare event known as “very late thermal pulse” (VLTP). To support our argument we compare the light curve of NSV 11749 with those of the two bona fide VLTP objects known to date, V4334 Sgr and V605 Aql, and with those predicted by state-of-the-art stellar evolution models. Next, we explore the INT Photometric H-Alpha Survey (IPHAS) and Two Micron All Sky Survey (2MASS) catalogs for possible counterparts of the eruption. Our analysis shows that the VLTP scenario outperforms all other proposed scenarios as an explanation of NSV 11749. We identify an IPHAS/2MASS source at the eruption location of NSV 11749. The derived colors suggest that the object is not enshrouded in a thick dust shell as V605 Aql and V4334 Sgr. Also, the absence of an apparent planetary nebula at the eruption location suggests differences with known VLTP objects which might be linked to the intensity of the eruption and the mass of the object. Further exploration of this source and scenario seems desirable. If NSV 11749 was a born-again star, it would be the third event of its kind to have been observed and will strongly help us to increase our understanding of the later stages of stellar evolution and violent reactive convective burning.
Fil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Rohrmann, R. D.. Consejo Nacional de Investigaciones Cientiâ­ficas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina
Fil: Granada, A.. Observatoire Astronomique de l’Universite de Genéeve; Suiza
Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
description We argue that NSV 11749, an eWe argue that NSV 11749, an eruption observed in the early twentieth century, was a rare event known as “very late thermal pulse” (VLTP). To support our argument we compare the light curve of NSV 11749 with those of the two bona fide VLTP objects known to date, V4334 Sgr and V605 Aql, and with those predicted by state-of-the-art stellar evolution models. Next, we explore the INT Photometric H-Alpha Survey (IPHAS) and Two Micron All Sky Survey (2MASS) catalogs for possible counterparts of the eruption. Our analysis shows that the VLTP scenario outperforms all other proposed scenarios as an explanation of NSV 11749. We identify an IPHAS/2MASS source at the eruption location of NSV 11749. The derived colors suggest that the object is not enshrouded in a thick dust shell as V605 Aql and V4334 Sgr. Also, the absence of an apparent planetary nebula at the eruption location suggests differences with known VLTP objects which might be linked to the intensity of the eruption and the mass of the object. Further exploration of this source and scenario seems desirable. If NSV 11749 was a born-again star, it would be the third event of its kind to have been observed and will strongly help us to increase our understanding of the later stages of stellar evolution and violent reactive convective burning.
publishDate 2011
dc.date.none.fl_str_mv 2011-12
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/11336/10084
Miller Bertolami, Marcelo Miguel; Rohrmann, R. D.; Granada, A.; Althaus, Leandro Gabriel; NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?; Iop Publishing; Astrophysical Journal; 743; 2; 12-2011; 1-6
0004-637X
url http://hdl.handle.net/11336/10084
identifier_str_mv Miller Bertolami, Marcelo Miguel; Rohrmann, R. D.; Granada, A.; Althaus, Leandro Gabriel; NSV 11749, an elder sibling of the born-again stars V605 Aql and V4334 Sgr?; Iop Publishing; Astrophysical Journal; 743; 2; 12-2011; 1-6
0004-637X
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/743/2/L33/meta
info:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/743/2/L33
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 Iop Publishing
publisher.none.fl_str_mv Iop Publishing
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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