Artículo

Symbiotic stars in X-rays II: Faint sources detected with XMM- Newton and Chandra

Nuñez, Natalia EdithIcon ; Luna, Gerardo Juan ManuelIcon ; Pilliteri, I.; Mukai, K.
Fecha de publicación: 05/2014
Editorial: EDP Sciences
Revista: Astronomy and Astrophysics
ISSN: 0004-6361
Idioma: Inglés
Tipo de recurso: Artículo publicado
Clasificación temática:

Resumen

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.
Palabras clave: Symbiotics , X-Ray
 
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info:eu-repo/semantics/openAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)
Identificadores
URI: http://hdl.handle.net/11336/4964
URL: http://www.aanda.org/articles/aa/abs/2014/05/aa22999-13/aa22999-13.html
DOI: http://dx.doi.org/10.1051/0004-6361/201322999
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Articulos(IAFE)
Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)
Articulos(ICATE)
Articulos de INST.D/CS ASTRONOMICAS D/LA TIERRA Y DEL ESPACIO
Citación
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
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