The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions

Astrometry (positions and proper motions) and photographic BVR photometry were determined from a set of 29 photographic plates and CCD data in a region of in the area of open clusters NGC 1750 and NGC 1758 in Taurus. The iterative central overlap algorithm was used for the proper motion calculations...

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Autores: Galadí-Enríquez, David, Jordi i Nebot, Carme, Trullols i Farreny, Enric, Guibert, J., Tian, K. P., Zhao, Junliang
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:1998
País:España
Institución:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
Repositorio:Recercat. Dipósit de la Recerca de Catalunya
OAI Identifier:oai:recercat.cat:2445/9207
Acceso en línea:https://hdl.handle.net/2445/9207
Access Level:acceso abierto
Palabra clave:Cúmuls de galàxies
Fotometria astronòmica
Astrometria
Open clusters and associations: individual: NGC 1746
Open clusters and associations: individual: NGC 1750
Open clusters and associations: individual: NGC 1758
Methods: astrometry
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spelling The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motionsGaladí-Enríquez, DavidJordi i Nebot, CarmeTrullols i Farreny, EnricGuibert, J.Tian, K. P.Zhao, JunliangCúmuls de galàxiesFotometria astronòmicaAstrometriaOpen clusters and associations: individual: NGC 1746Open clusters and associations: individual: NGC 1750Open clusters and associations: individual: NGC 1758Methods: astrometryAstrometry (positions and proper motions) and photographic BVR photometry were determined from a set of 29 photographic plates and CCD data in a region of in the area of open clusters NGC 1750 and NGC 1758 in Taurus. The iterative central overlap algorithm was used for the proper motion calculations. Plate-to-plate transformations and astrometric magnitude effects are discussed in detail. CCD data interact with photographic material in three different ways: for the elimination of astrometric magnitude effects, for the photometric standard calibration of photographic plates and for building a CCD pseudo-plate used for astrometric purposes as any other photographic plate. A preliminary analysis of the resulting photometric and astrometric catalogue confirmed the reality of two different clusters in the zone (NGC 1750 and NGC 1758). There were no indications for the existence of NGC 1746.EDP Sciences200920091998info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersion20 p.application/pdfhttps://hdl.handle.net/2445/9207Articles publicats en revistes (Física Quàntica i Astrofísica)reponame:Recercat. Dipósit de la Recerca de Catalunyainstname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)InglésReproducció del document publicat a http://dx.doi.org/10.1051/aas:1998433Astronomy and Astrophysics Supplement Series, 1998, vol. 131, núm. 2, p. 239-258.http://dx.doi.org/10.1051/aas:1998433(c) The European Southern Observatory, 1998info:eu-repo/semantics/openAccessoai:recercat.cat:2445/92072026-05-29T05:05:01Z
dc.title.none.fl_str_mv The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions
title The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions
spellingShingle The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions
Galadí-Enríquez, David
Cúmuls de galàxies
Fotometria astronòmica
Astrometria
Open clusters and associations: individual: NGC 1746
Open clusters and associations: individual: NGC 1750
Open clusters and associations: individual: NGC 1758
Methods: astrometry
title_short The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions
title_full The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions
title_fullStr The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions
title_full_unstemmed The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions
title_sort The overlapping open clusters NGC 1750 and NGC 1758 II. BV R photographic photometry and proper motions
dc.creator.none.fl_str_mv Galadí-Enríquez, David
Jordi i Nebot, Carme
Trullols i Farreny, Enric
Guibert, J.
Tian, K. P.
Zhao, Junliang
author Galadí-Enríquez, David
author_facet Galadí-Enríquez, David
Jordi i Nebot, Carme
Trullols i Farreny, Enric
Guibert, J.
Tian, K. P.
Zhao, Junliang
author_role author
author2 Jordi i Nebot, Carme
Trullols i Farreny, Enric
Guibert, J.
Tian, K. P.
Zhao, Junliang
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Cúmuls de galàxies
Fotometria astronòmica
Astrometria
Open clusters and associations: individual: NGC 1746
Open clusters and associations: individual: NGC 1750
Open clusters and associations: individual: NGC 1758
Methods: astrometry
topic Cúmuls de galàxies
Fotometria astronòmica
Astrometria
Open clusters and associations: individual: NGC 1746
Open clusters and associations: individual: NGC 1750
Open clusters and associations: individual: NGC 1758
Methods: astrometry
description Astrometry (positions and proper motions) and photographic BVR photometry were determined from a set of 29 photographic plates and CCD data in a region of in the area of open clusters NGC 1750 and NGC 1758 in Taurus. The iterative central overlap algorithm was used for the proper motion calculations. Plate-to-plate transformations and astrometric magnitude effects are discussed in detail. CCD data interact with photographic material in three different ways: for the elimination of astrometric magnitude effects, for the photometric standard calibration of photographic plates and for building a CCD pseudo-plate used for astrometric purposes as any other photographic plate. A preliminary analysis of the resulting photometric and astrometric catalogue confirmed the reality of two different clusters in the zone (NGC 1750 and NGC 1758). There were no indications for the existence of NGC 1746.
publishDate 1998
dc.date.none.fl_str_mv 1998
2009
2009
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://hdl.handle.net/2445/9207
url https://hdl.handle.net/2445/9207
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv Reproducció del document publicat a http://dx.doi.org/10.1051/aas:1998433
Astronomy and Astrophysics Supplement Series, 1998, vol. 131, núm. 2, p. 239-258.
http://dx.doi.org/10.1051/aas:1998433
dc.rights.none.fl_str_mv (c) The European Southern Observatory, 1998
info:eu-repo/semantics/openAccess
rights_invalid_str_mv (c) The European Southern Observatory, 1998
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 20 p.
application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv Articles publicats en revistes (Física Quàntica i Astrofísica)
reponame:Recercat. Dipósit de la Recerca de Catalunya
instname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
instname_str Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
reponame_str Recercat. Dipósit de la Recerca de Catalunya
collection Recercat. Dipósit de la Recerca de Catalunya
repository.name.fl_str_mv
repository.mail.fl_str_mv
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