On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula

Autores
Majaess, D.; Carraro, G.; Moni Bidin, C.; Bonatto, C.; Turner, D.; Moyano, M.; Berdnikov, L.; Giorgi, Edgard Ervar Salvador
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Andrews-Lindsay 1 is a pertinent open cluster because it may host the planetary nebula (PN) PHR 1315-6555, yet ambiguities linger concerning its fundamental parameters (>50% scatter). New multiband BVJHW1 - 4 photometry for cluster and field stars, in concert with observations of recently discovered classical Cepheids, were used to constrain the reddening and velocity-distance profiles along the sightline. That analysis yielded the following parameters for the cluster: E(J - H) = 0.24 ± 0.03, d = 10.0 ± 0.4 kpc (dJH = 9.9 ± 0.6 kpc, dBV = 10.1 ± 0.5 kpc), and log τ = 8.90 ± 0.15. The steep velocity-distance gradient along ℓ ∼ 305° indicates that two remote objects sharing spatial and kinematic parameters (i.e., PHR 1315-6555 and Andrews-Lindsay 1) are associated, thus confirming claims that the PN is a cluster member. The new distance for PHR 1315-6555 is among the most precise established yet for a Galactic PN (σ/d = 4%).
Instituto de Astrofísica de La Plata
Materia
Ciencias Astronómicas
Open clusters and associations: individual: Andrews-Lindsay 1 (ESO 96-SC04)
Planetary nebulae: individual: PHR 1315-6555
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/85374

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network_name_str SEDICI (UNLP)
spelling On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebulaMajaess, D.Carraro, G.Moni Bidin, C.Bonatto, C.Turner, D.Moyano, M.Berdnikov, L.Giorgi, Edgard Ervar SalvadorCiencias AstronómicasOpen clusters and associations: individual: Andrews-Lindsay 1 (ESO 96-SC04)Planetary nebulae: individual: PHR 1315-6555Andrews-Lindsay 1 is a pertinent open cluster because it may host the planetary nebula (PN) PHR 1315-6555, yet ambiguities linger concerning its fundamental parameters (>50% scatter). New multiband BVJHW1 - 4 photometry for cluster and field stars, in concert with observations of recently discovered classical Cepheids, were used to constrain the reddening and velocity-distance profiles along the sightline. That analysis yielded the following parameters for the cluster: E(J - H) = 0.24 ± 0.03, d = 10.0 ± 0.4 kpc (dJH = 9.9 ± 0.6 kpc, dBV = 10.1 ± 0.5 kpc), and log τ = 8.90 ± 0.15. The steep velocity-distance gradient along ℓ ∼ 305° indicates that two remote objects sharing spatial and kinematic parameters (i.e., PHR 1315-6555 and Andrews-Lindsay 1) are associated, thus confirming claims that the PN is a cluster member. The new distance for PHR 1315-6555 is among the most precise established yet for a Galactic PN (σ/d = 4%).Instituto de Astrofísica de La Plata2014-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/85374enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201423673info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:16:25Zoai:sedici.unlp.edu.ar:10915/85374Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:26.091SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
title On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
spellingShingle On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
Majaess, D.
Ciencias Astronómicas
Open clusters and associations: individual: Andrews-Lindsay 1 (ESO 96-SC04)
Planetary nebulae: individual: PHR 1315-6555
title_short On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
title_full On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
title_fullStr On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
title_full_unstemmed On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
title_sort On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
dc.creator.none.fl_str_mv Majaess, D.
Carraro, G.
Moni Bidin, C.
Bonatto, C.
Turner, D.
Moyano, M.
Berdnikov, L.
Giorgi, Edgard Ervar Salvador
author Majaess, D.
author_facet Majaess, D.
Carraro, G.
Moni Bidin, C.
Bonatto, C.
Turner, D.
Moyano, M.
Berdnikov, L.
Giorgi, Edgard Ervar Salvador
author_role author
author2 Carraro, G.
Moni Bidin, C.
Bonatto, C.
Turner, D.
Moyano, M.
Berdnikov, L.
Giorgi, Edgard Ervar Salvador
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Open clusters and associations: individual: Andrews-Lindsay 1 (ESO 96-SC04)
Planetary nebulae: individual: PHR 1315-6555
topic Ciencias Astronómicas
Open clusters and associations: individual: Andrews-Lindsay 1 (ESO 96-SC04)
Planetary nebulae: individual: PHR 1315-6555
dc.description.none.fl_txt_mv Andrews-Lindsay 1 is a pertinent open cluster because it may host the planetary nebula (PN) PHR 1315-6555, yet ambiguities linger concerning its fundamental parameters (>50% scatter). New multiband BVJHW1 - 4 photometry for cluster and field stars, in concert with observations of recently discovered classical Cepheids, were used to constrain the reddening and velocity-distance profiles along the sightline. That analysis yielded the following parameters for the cluster: E(J - H) = 0.24 ± 0.03, d = 10.0 ± 0.4 kpc (dJH = 9.9 ± 0.6 kpc, dBV = 10.1 ± 0.5 kpc), and log τ = 8.90 ± 0.15. The steep velocity-distance gradient along ℓ ∼ 305° indicates that two remote objects sharing spatial and kinematic parameters (i.e., PHR 1315-6555 and Andrews-Lindsay 1) are associated, thus confirming claims that the PN is a cluster member. The new distance for PHR 1315-6555 is among the most precise established yet for a Galactic PN (σ/d = 4%).
Instituto de Astrofísica de La Plata
description Andrews-Lindsay 1 is a pertinent open cluster because it may host the planetary nebula (PN) PHR 1315-6555, yet ambiguities linger concerning its fundamental parameters (>50% scatter). New multiband BVJHW1 - 4 photometry for cluster and field stars, in concert with observations of recently discovered classical Cepheids, were used to constrain the reddening and velocity-distance profiles along the sightline. That analysis yielded the following parameters for the cluster: E(J - H) = 0.24 ± 0.03, d = 10.0 ± 0.4 kpc (dJH = 9.9 ± 0.6 kpc, dBV = 10.1 ± 0.5 kpc), and log τ = 8.90 ± 0.15. The steep velocity-distance gradient along ℓ ∼ 305° indicates that two remote objects sharing spatial and kinematic parameters (i.e., PHR 1315-6555 and Andrews-Lindsay 1) are associated, thus confirming claims that the PN is a cluster member. The new distance for PHR 1315-6555 is among the most precise established yet for a Galactic PN (σ/d = 4%).
publishDate 2014
dc.date.none.fl_str_mv 2014-07
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/85374
url http://sedici.unlp.edu.ar/handle/10915/85374
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0004-6361
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201423673
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
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repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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