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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/22324
Ver los metadatos del registro completo
id |
CONICETDig_97b2b6f06b70bffa664a77961b4b6da4 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/22324 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
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 Técnicas2025-09-29T10:14:49Zoai: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:34982025-09-29 10:14:49.757CONICET 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 |
_version_ |
1844614079680872448 |
score |
13.070432 |