A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars
- Autores
- Cappa, Cristina Elisabeth; Goss, William Miller; van der Hucht, K. A.
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We report the results of a survey of radio continuum emission of Galactic Wolf-Rayet (WR) stars north of δ = -46°. The observations were obtained at 8.46 GHz (3.6 cm) using the Very Large Array, with an angular resolution of ∼6″ × 9″ and typical rms noise of ∼0.04 mJy beam -1 . Our survey of 34 WR stars resulted in 15 definite, and five probable detections, 13 of these for the first time at radio wavelengths. All detections are unresolved (θ ≲ 5″). Time variations in flux are confirmed in the cases of WR 98a, 104, 105, and 125. WR 79a and WR 89 are also variable in flux, and we suspect they are also nonthermal emitters. Thus, of our sample 20%30% of the detected stars are nonthermal emitters. Average mass-loss rate determinations obtained excluding definite and suspected nonthermal cases give similar values for WN (all subtypes) and WC5-7 stars [M(WN) = (4 ± 3) × 10 -5 M ⊙ yr -1 and M(WC5-7) = (4 ± 2) × 10 -5 M× yr -1 ], while a lower value was obtained for WC8-9 stars [M(WC8-9) = (2 ± 1) × 10 -5 M ⊙ yr -1 ]. Uncertainties in stellar distances largely contribute to the observed scatter in mass-loss rates. Upper limits to the mass-loss rates were obtained in cases of undetected sources and for sources that probably show additional nonthermal emission.
Fil: Cappa, Cristina Elisabeth. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Goss, William Miller. National Radio Astronomy Observatory; Estados Unidos
Fil: van der Hucht, K. A.. Sron Netherlands Institute For Space Research; Países Bajos - Materia
-
STELLAR WINDS
WR STARS - 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:11336/76343
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oai:ri.conicet.gov.ar:11336/76343 |
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3498 |
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CONICET Digital (CONICET) |
spelling |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet starsCappa, Cristina ElisabethGoss, William Millervan der Hucht, K. A.STELLAR WINDSWR STARSWe report the results of a survey of radio continuum emission of Galactic Wolf-Rayet (WR) stars north of δ = -46°. The observations were obtained at 8.46 GHz (3.6 cm) using the Very Large Array, with an angular resolution of ∼6″ × 9″ and typical rms noise of ∼0.04 mJy beam -1 . Our survey of 34 WR stars resulted in 15 definite, and five probable detections, 13 of these for the first time at radio wavelengths. All detections are unresolved (θ ≲ 5″). Time variations in flux are confirmed in the cases of WR 98a, 104, 105, and 125. WR 79a and WR 89 are also variable in flux, and we suspect they are also nonthermal emitters. Thus, of our sample 20%30% of the detected stars are nonthermal emitters. Average mass-loss rate determinations obtained excluding definite and suspected nonthermal cases give similar values for WN (all subtypes) and WC5-7 stars [M(WN) = (4 ± 3) × 10 -5 M ⊙ yr -1 and M(WC5-7) = (4 ± 2) × 10 -5 M× yr -1 ], while a lower value was obtained for WC8-9 stars [M(WC8-9) = (2 ± 1) × 10 -5 M ⊙ yr -1 ]. Uncertainties in stellar distances largely contribute to the observed scatter in mass-loss rates. Upper limits to the mass-loss rates were obtained in cases of undetected sources and for sources that probably show additional nonthermal emission.Fil: Cappa, Cristina Elisabeth. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Goss, William Miller. National Radio Astronomy Observatory; Estados UnidosFil: van der Hucht, K. A.. Sron Netherlands Institute For Space Research; Países BajosIOP Publishing2004-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/76343Cappa, Cristina Elisabeth; Goss, William Miller; van der Hucht, K. A. ; A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars; IOP Publishing; Astronomical Journal; 127; 5; 6-2004; 2885-28970004-6256CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1086/383286info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/383286/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:14:05Zoai:ri.conicet.gov.ar:11336/76343instacron: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 10:14:06.216CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars |
title |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars |
spellingShingle |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars Cappa, Cristina Elisabeth STELLAR WINDS WR STARS |
title_short |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars |
title_full |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars |
title_fullStr |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars |
title_full_unstemmed |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars |
title_sort |
A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars |
dc.creator.none.fl_str_mv |
Cappa, Cristina Elisabeth Goss, William Miller van der Hucht, K. A. |
author |
Cappa, Cristina Elisabeth |
author_facet |
Cappa, Cristina Elisabeth Goss, William Miller van der Hucht, K. A. |
author_role |
author |
author2 |
Goss, William Miller van der Hucht, K. A. |
author2_role |
author author |
dc.subject.none.fl_str_mv |
STELLAR WINDS WR STARS |
topic |
STELLAR WINDS WR STARS |
dc.description.none.fl_txt_mv |
We report the results of a survey of radio continuum emission of Galactic Wolf-Rayet (WR) stars north of δ = -46°. The observations were obtained at 8.46 GHz (3.6 cm) using the Very Large Array, with an angular resolution of ∼6″ × 9″ and typical rms noise of ∼0.04 mJy beam -1 . Our survey of 34 WR stars resulted in 15 definite, and five probable detections, 13 of these for the first time at radio wavelengths. All detections are unresolved (θ ≲ 5″). Time variations in flux are confirmed in the cases of WR 98a, 104, 105, and 125. WR 79a and WR 89 are also variable in flux, and we suspect they are also nonthermal emitters. Thus, of our sample 20%30% of the detected stars are nonthermal emitters. Average mass-loss rate determinations obtained excluding definite and suspected nonthermal cases give similar values for WN (all subtypes) and WC5-7 stars [M(WN) = (4 ± 3) × 10 -5 M ⊙ yr -1 and M(WC5-7) = (4 ± 2) × 10 -5 M× yr -1 ], while a lower value was obtained for WC8-9 stars [M(WC8-9) = (2 ± 1) × 10 -5 M ⊙ yr -1 ]. Uncertainties in stellar distances largely contribute to the observed scatter in mass-loss rates. Upper limits to the mass-loss rates were obtained in cases of undetected sources and for sources that probably show additional nonthermal emission. Fil: Cappa, Cristina Elisabeth. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Goss, William Miller. National Radio Astronomy Observatory; Estados Unidos Fil: van der Hucht, K. A.. Sron Netherlands Institute For Space Research; Países Bajos |
description |
We report the results of a survey of radio continuum emission of Galactic Wolf-Rayet (WR) stars north of δ = -46°. The observations were obtained at 8.46 GHz (3.6 cm) using the Very Large Array, with an angular resolution of ∼6″ × 9″ and typical rms noise of ∼0.04 mJy beam -1 . Our survey of 34 WR stars resulted in 15 definite, and five probable detections, 13 of these for the first time at radio wavelengths. All detections are unresolved (θ ≲ 5″). Time variations in flux are confirmed in the cases of WR 98a, 104, 105, and 125. WR 79a and WR 89 are also variable in flux, and we suspect they are also nonthermal emitters. Thus, of our sample 20%30% of the detected stars are nonthermal emitters. Average mass-loss rate determinations obtained excluding definite and suspected nonthermal cases give similar values for WN (all subtypes) and WC5-7 stars [M(WN) = (4 ± 3) × 10 -5 M ⊙ yr -1 and M(WC5-7) = (4 ± 2) × 10 -5 M× yr -1 ], while a lower value was obtained for WC8-9 stars [M(WC8-9) = (2 ± 1) × 10 -5 M ⊙ yr -1 ]. Uncertainties in stellar distances largely contribute to the observed scatter in mass-loss rates. Upper limits to the mass-loss rates were obtained in cases of undetected sources and for sources that probably show additional nonthermal emission. |
publishDate |
2004 |
dc.date.none.fl_str_mv |
2004-06 |
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/11336/76343 Cappa, Cristina Elisabeth; Goss, William Miller; van der Hucht, K. A. ; A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars; IOP Publishing; Astronomical Journal; 127; 5; 6-2004; 2885-2897 0004-6256 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/76343 |
identifier_str_mv |
Cappa, Cristina Elisabeth; Goss, William Miller; van der Hucht, K. A. ; A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars; IOP Publishing; Astronomical Journal; 127; 5; 6-2004; 2885-2897 0004-6256 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1086/383286 info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/383286/meta |
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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1844614064514269184 |
score |
13.070432 |