Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra
- Autores
- Nuñez, Natalia Edith; Luna, Gerardo Juan Manuel; Pilliteri, I.; Mukai, K.
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We report the detection from four symbiotics stars that were not known to be X-ray sources. These four object show a beta-type X-ray spectrum, that is, their spectra can be modeled with an absorbed optically thin thermal emission with temperatures of a few million degrees. Photometric series obtained with the Optical Monitor on board XMM- Newton from V2416 Sgr and NSV 25735 support the proposed scenario where the X-ray emission is produced in a shock-heated region inside the symbiotic nebulae.
Fil: Nuñez, Natalia Edith. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina
Fil: Luna, Gerardo Juan Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio(i); Argentina
Fil: Pilliteri, I.. Osservatorio Astronomico di Palermo; Italia
Fil: Mukai, K.. University of Maryland. Department of Physics. CRESST and X-ray Astrophysics Laboratory; Estados Unidos - Materia
-
SYMBIOTICS
X-RAY - 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:11336/4964
Ver los metadatos del registro completo
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Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and ChandraNuñez, Natalia EdithLuna, Gerardo Juan ManuelPilliteri, I.Mukai, K.SYMBIOTICSX-RAYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We report the detection from four symbiotics stars that were not known to be X-ray sources. These four object show a beta-type X-ray spectrum, that is, their spectra can be modeled with an absorbed optically thin thermal emission with temperatures of a few million degrees. Photometric series obtained with the Optical Monitor on board XMM- Newton from V2416 Sgr and NSV 25735 support the proposed scenario where the X-ray emission is produced in a shock-heated region inside the symbiotic nebulae.Fil: Nuñez, Natalia Edith. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; ArgentinaFil: Luna, Gerardo Juan Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio(i); ArgentinaFil: Pilliteri, I.. Osservatorio Astronomico di Palermo; ItaliaFil: Mukai, K.. University of Maryland. Department of Physics. CRESST and X-ray Astrophysics Laboratory; Estados UnidosEDP Sciences2014-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/4964Nuñez, Natalia Edith; Luna, Gerardo Juan Manuel; Pilliteri, I.; Mukai, K.; Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra; EDP Sciences; Astronomy and Astrophysics; 565; 5-2014; 82-860004-6361enginfo:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2014/05/aa22999-13/aa22999-13.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201322999info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:44:47Zoai:ri.conicet.gov.ar:11336/4964instacron: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 09:44:47.917CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra |
title |
Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra |
spellingShingle |
Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra Nuñez, Natalia Edith SYMBIOTICS X-RAY |
title_short |
Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra |
title_full |
Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra |
title_fullStr |
Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra |
title_full_unstemmed |
Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra |
title_sort |
Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra |
dc.creator.none.fl_str_mv |
Nuñez, Natalia Edith Luna, Gerardo Juan Manuel Pilliteri, I. Mukai, K. |
author |
Nuñez, Natalia Edith |
author_facet |
Nuñez, Natalia Edith Luna, Gerardo Juan Manuel Pilliteri, I. Mukai, K. |
author_role |
author |
author2 |
Luna, Gerardo Juan Manuel Pilliteri, I. Mukai, K. |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
SYMBIOTICS X-RAY |
topic |
SYMBIOTICS X-RAY |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We report the detection from four symbiotics stars that were not known to be X-ray sources. These four object show a beta-type X-ray spectrum, that is, their spectra can be modeled with an absorbed optically thin thermal emission with temperatures of a few million degrees. Photometric series obtained with the Optical Monitor on board XMM- Newton from V2416 Sgr and NSV 25735 support the proposed scenario where the X-ray emission is produced in a shock-heated region inside the symbiotic nebulae. Fil: Nuñez, Natalia Edith. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina Fil: Luna, Gerardo Juan Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio(i); Argentina Fil: Pilliteri, I.. Osservatorio Astronomico di Palermo; Italia Fil: Mukai, K.. University of Maryland. Department of Physics. CRESST and X-ray Astrophysics Laboratory; Estados Unidos |
description |
We report the detection from four symbiotics stars that were not known to be X-ray sources. These four object show a beta-type X-ray spectrum, that is, their spectra can be modeled with an absorbed optically thin thermal emission with temperatures of a few million degrees. Photometric series obtained with the Optical Monitor on board XMM- Newton from V2416 Sgr and NSV 25735 support the proposed scenario where the X-ray emission is produced in a shock-heated region inside the symbiotic nebulae. |
publishDate |
2014 |
dc.date.none.fl_str_mv |
2014-05 |
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/11336/4964 Nuñez, Natalia Edith; Luna, Gerardo Juan Manuel; Pilliteri, I.; Mukai, K.; Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra; EDP Sciences; Astronomy and Astrophysics; 565; 5-2014; 82-86 0004-6361 |
url |
http://hdl.handle.net/11336/4964 |
identifier_str_mv |
Nuñez, Natalia Edith; Luna, Gerardo Juan Manuel; Pilliteri, I.; Mukai, K.; Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra; EDP Sciences; Astronomy and Astrophysics; 565; 5-2014; 82-86 0004-6361 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2014/05/aa22999-13/aa22999-13.html info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201322999 |
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 |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
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 |
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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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1844613409637662720 |
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13.070432 |