On the distance and structure of W80

Autores
Cersósimo, Juan Carlos; Muller, R. J.; Figueroa Vélez, S.; Santiago Figueroa, N.; Baez, P.; Testori, Juan Carlos
Año de publicación
2007
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The continuum radiation of the Galactic region located at l = 85°, b = -0.5° is well defined by its 11 cm emission. The region, extended 3° in diameter, is cataloged as W80, and its optical images show the North America and Pelican Nebulae complexes. In this paper we present new distance measurements and physical parameters obtained from radio recombination line observations at a frequency near 1.4 GHz. Four structures are identified in the region under study: a near structure is located at a distance of about 0.7 kpc, another structure lies on the east side of W80 at a distance of 1.7 kpc, there is a concentration of ionized gas on the west side at a distance of 2.7 kpc, and a fourth structure is found further away at 3.3 kpc, which does not seem to belong to the W80 complex. The results are presented using the (X, Y, Z)-coordinates of the Galactic plane. The model used assumes a constant electron temperature Te = 6800 K and also assumes homogeneity. Our results seem to indicate that the ionized hydrogen of W80 spreads along the line of sight instead of clumping at one distance. We obtain values of the electron density and the ionization parameter between ne = 5 and 16 cm-3 and U = 51 and 110 cm-2 pc, respectively.
Fil: Cersósimo, Juan Carlos. Universidad de Puerto Rico; Puerto Rico
Fil: Muller, R. J.. Universidad de Puerto Rico; Puerto Rico
Fil: Figueroa Vélez, S.. Universidad de Puerto Rico; Puerto Rico
Fil: Santiago Figueroa, N.. Universidad de Puerto Rico; Puerto Rico
Fil: Baez, P.. Universidad de Puerto Rico; Puerto Rico
Fil: Testori, Juan Carlos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
Materia
Radio Continuum
Hii Regions
Interstellar Medium
W80 (Estrella)
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:11336/22324
Acceder
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network_name_str CONICET Digital (CONICET)
spelling On the distance and structure of W80Cersósimo, Juan CarlosMuller, R. J.Figueroa Vélez, S.Santiago Figueroa, N.Baez, P.Testori, Juan CarlosRadio ContinuumHii RegionsInterstellar MediumW80 (Estrella)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The continuum radiation of the Galactic region located at l = 85°, b = -0.5° is well defined by its 11 cm emission. The region, extended 3° in diameter, is cataloged as W80, and its optical images show the North America and Pelican Nebulae complexes. In this paper we present new distance measurements and physical parameters obtained from radio recombination line observations at a frequency near 1.4 GHz. Four structures are identified in the region under study: a near structure is located at a distance of about 0.7 kpc, another structure lies on the east side of W80 at a distance of 1.7 kpc, there is a concentration of ionized gas on the west side at a distance of 2.7 kpc, and a fourth structure is found further away at 3.3 kpc, which does not seem to belong to the W80 complex. The results are presented using the (X, Y, Z)-coordinates of the Galactic plane. The model used assumes a constant electron temperature Te = 6800 K and also assumes homogeneity. Our results seem to indicate that the ionized hydrogen of W80 spreads along the line of sight instead of clumping at one distance. We obtain values of the electron density and the ionization parameter between ne = 5 and 16 cm-3 and U = 51 and 110 cm-2 pc, respectively.Fil: Cersósimo, Juan Carlos. Universidad de Puerto Rico; Puerto RicoFil: Muller, R. J.. Universidad de Puerto Rico; Puerto RicoFil: Figueroa Vélez, S.. Universidad de Puerto Rico; Puerto RicoFil: Santiago Figueroa, N.. Universidad de Puerto Rico; Puerto RicoFil: Baez, P.. Universidad de Puerto Rico; Puerto RicoFil: Testori, Juan Carlos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; ArgentinaIop Publishing2007-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/22324Cersósimo, Juan Carlos; Muller, R. J.; Figueroa Vélez, S.; Santiago Figueroa, N.; Baez, P.; et al.; On the distance and structure of W80; Iop Publishing; Astrophysical Journal; 656; 1; 12-2007; 248-2540004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2007ApJ...656..248Cinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/510372/metainfo:eu-repo/semantics/altIdentifier/doi/10.1086/510372info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:12:03Zoai:ri.conicet.gov.ar:11336/22324instacron: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:34982025-10-15 15:12:04.03CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv On the distance and structure of W80
title On the distance and structure of W80
spellingShingle On the distance and structure of W80
Cersósimo, Juan Carlos
Radio Continuum
Hii Regions
Interstellar Medium
W80 (Estrella)
title_short On the distance and structure of W80
title_full On the distance and structure of W80
title_fullStr On the distance and structure of W80
title_full_unstemmed On the distance and structure of W80
title_sort On the distance and structure of W80
dc.creator.none.fl_str_mv Cersósimo, Juan Carlos
Muller, R. J.
Figueroa Vélez, S.
Santiago Figueroa, N.
Baez, P.
Testori, Juan Carlos
author Cersósimo, Juan Carlos
author_facet Cersósimo, Juan Carlos
Muller, R. J.
Figueroa Vélez, S.
Santiago Figueroa, N.
Baez, P.
Testori, Juan Carlos
author_role author
author2 Muller, R. J.
Figueroa Vélez, S.
Santiago Figueroa, N.
Baez, P.
Testori, Juan Carlos
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Radio Continuum
Hii Regions
Interstellar Medium
W80 (Estrella)
topic Radio Continuum
Hii Regions
Interstellar Medium
W80 (Estrella)
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 continuum radiation of the Galactic region located at l = 85°, b = -0.5° is well defined by its 11 cm emission. The region, extended 3° in diameter, is cataloged as W80, and its optical images show the North America and Pelican Nebulae complexes. In this paper we present new distance measurements and physical parameters obtained from radio recombination line observations at a frequency near 1.4 GHz. Four structures are identified in the region under study: a near structure is located at a distance of about 0.7 kpc, another structure lies on the east side of W80 at a distance of 1.7 kpc, there is a concentration of ionized gas on the west side at a distance of 2.7 kpc, and a fourth structure is found further away at 3.3 kpc, which does not seem to belong to the W80 complex. The results are presented using the (X, Y, Z)-coordinates of the Galactic plane. The model used assumes a constant electron temperature Te = 6800 K and also assumes homogeneity. Our results seem to indicate that the ionized hydrogen of W80 spreads along the line of sight instead of clumping at one distance. We obtain values of the electron density and the ionization parameter between ne = 5 and 16 cm-3 and U = 51 and 110 cm-2 pc, respectively.
Fil: Cersósimo, Juan Carlos. Universidad de Puerto Rico; Puerto Rico
Fil: Muller, R. J.. Universidad de Puerto Rico; Puerto Rico
Fil: Figueroa Vélez, S.. Universidad de Puerto Rico; Puerto Rico
Fil: Santiago Figueroa, N.. Universidad de Puerto Rico; Puerto Rico
Fil: Baez, P.. Universidad de Puerto Rico; Puerto Rico
Fil: Testori, Juan Carlos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
description The continuum radiation of the Galactic region located at l = 85°, b = -0.5° is well defined by its 11 cm emission. The region, extended 3° in diameter, is cataloged as W80, and its optical images show the North America and Pelican Nebulae complexes. In this paper we present new distance measurements and physical parameters obtained from radio recombination line observations at a frequency near 1.4 GHz. Four structures are identified in the region under study: a near structure is located at a distance of about 0.7 kpc, another structure lies on the east side of W80 at a distance of 1.7 kpc, there is a concentration of ionized gas on the west side at a distance of 2.7 kpc, and a fourth structure is found further away at 3.3 kpc, which does not seem to belong to the W80 complex. The results are presented using the (X, Y, Z)-coordinates of the Galactic plane. The model used assumes a constant electron temperature Te = 6800 K and also assumes homogeneity. Our results seem to indicate that the ionized hydrogen of W80 spreads along the line of sight instead of clumping at one distance. We obtain values of the electron density and the ionization parameter between ne = 5 and 16 cm-3 and U = 51 and 110 cm-2 pc, respectively.
publishDate 2007
dc.date.none.fl_str_mv 2007-12
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/11336/22324
Cersósimo, Juan Carlos; Muller, R. J.; Figueroa Vélez, S.; Santiago Figueroa, N.; Baez, P.; et al.; On the distance and structure of W80; Iop Publishing; Astrophysical Journal; 656; 1; 12-2007; 248-254
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/22324
identifier_str_mv Cersósimo, Juan Carlos; Muller, R. J.; Figueroa Vélez, S.; Santiago Figueroa, N.; Baez, P.; et al.; On the distance and structure of W80; Iop Publishing; Astrophysical Journal; 656; 1; 12-2007; 248-254
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2007ApJ...656..248C
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/510372/meta
info:eu-repo/semantics/altIdentifier/doi/10.1086/510372
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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score 13.22299

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