Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra
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 wi...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v565_n_p_Nunez |
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todo:paper_00046361_v565_n_p_Nunez2023-10-03T14:00:50Z Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra Nuñez, N.E. Luna, G.J.M. Pillitteri, I. Mukai, K. 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 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. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00046361_v565_n_p_Nunez |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
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 |
spellingShingle |
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 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 |
topic_facet |
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 |
description |
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. |
format |
JOUR |
author |
Nuñez, N.E. Luna, G.J.M. Pillitteri, I. Mukai, K. |
author_facet |
Nuñez, N.E. Luna, G.J.M. Pillitteri, I. Mukai, K. |
author_sort |
Nuñez, N.E. |
title |
Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra |
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 |
url |
http://hdl.handle.net/20.500.12110/paper_00046361_v565_n_p_Nunez |
work_keys_str_mv |
AT nunezne symbioticstarsinxraysiifaintsourcesdetectedwithxmmnewtonandchandra AT lunagjm symbioticstarsinxraysiifaintsourcesdetectedwithxmmnewtonandchandra AT pillitterii symbioticstarsinxraysiifaintsourcesdetectedwithxmmnewtonandchandra AT mukaik symbioticstarsinxraysiifaintsourcesdetectedwithxmmnewtonandchandra |
_version_ |
1807318445751009280 |