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Abstract:

We report the detection from four symbiotic stars that were not known to be X-ray sources. These four object show a β-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. © 2014 ESO.

Registro:

Documento: Artículo
Título:Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra
Autor:Nuñez, N.E.; Luna, G.J.M.; Pillitteri, I.; Mukai, K.
Filiación:Instituto de Ciencias Astronómicas de la Tierra y El Espacio ICATE, UNSJ, Av. España (sur) 1512, 5400 San Juan, Argentina
Instituto de Astronomía y Física Del Espacio (IAFE), CC 67, C1428ZAA Caba, Argentina
Osservatorio Astronomico di Palermo (INAF), piazza del Parlamento 1, 90 134 Palermo, Italy
CRESST, X-ray Astrophysics Laboratory, NASA, Greenbelt MD 20 771, United States
Department of Physics, University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore MD 21 250, United States
Palabras clave:Binaries: symbiotic; X-rays: binaries; Stars; X ray optics; Binaries: symbiotic; Optical monitors; Symbiotic stars; Thermal emissions; X ray spectrum; X-ray emission; X-ray sources; X-rays: Binaries; X rays
Año:2014
Volumen:565
DOI: http://dx.doi.org/10.1051/0004-6361/201322999
Título revista:Astronomy and Astrophysics
Título revista abreviado:Astron. Astrophys.
ISSN:00046361
CODEN:AAEJA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v565_n_p_Nunez

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Citas:

---------- APA ----------
Nuñez, N.E., Luna, G.J.M., Pillitteri, I. & Mukai, K. (2014) . Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra. Astronomy and Astrophysics, 565.
http://dx.doi.org/10.1051/0004-6361/201322999
---------- CHICAGO ----------
Nuñez, N.E., Luna, G.J.M., Pillitteri, I., Mukai, K. "Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra" . Astronomy and Astrophysics 565 (2014).
http://dx.doi.org/10.1051/0004-6361/201322999
---------- MLA ----------
Nuñez, N.E., Luna, G.J.M., Pillitteri, I., Mukai, K. "Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra" . Astronomy and Astrophysics, vol. 565, 2014.
http://dx.doi.org/10.1051/0004-6361/201322999
---------- VANCOUVER ----------
Nuñez, N.E., Luna, G.J.M., Pillitteri, I., Mukai, K. Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra. Astron. Astrophys. 2014;565.
http://dx.doi.org/10.1051/0004-6361/201322999