Peering into the central region of a nano-quasar: XMM-Newton and Chandra views of the CH Cyg Symbiotic System

Abstract

We present the analysis of archival XMM-Newton and Chandra observations of CH Cyg, one of the most studied symbiotic stars (SySts). The combination of the high-resolution XMM-Newton RGS and Chandra HETG X-ray spectra allowed us to obtain reliable estimates of the chemical abundances and to corroborate the presence of multi-temperature X-ray-emitting gas. Spectral fitting of the medium-resolution XMM-Newton MOS (MOS1+MOS2) spectrum required the use of an additional component not seen in previous studies in order to fit the 2.0-4.0 keV energy range. Detailed spectral modelling of the XMM-Newton MOS data suggests the presence of a reflection component, very similar to that found in active galactic nuclei. The reflection component is very likely produced by an ionised disk (the accretion disk around the white dwarf) and naturally explains the presence of the fluorescent Fe emission line at 6.4 keV while also contributing to the soft and medium energy ranges. The variability of the global X-ray properties of CH Cyg are discussed as well as the variation of the three Fe lines around the 6-7 keV energy range. We conclude that reflection components are needed to model the hard X-ray emission and may be present in most $\beta /\delta$-type SySt.

12 pages, 7 figures, 5 tables; To appear in MNRAS

References in corpus (9)

• Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3
• RefleX: X-ray absorption and reflection in active galactic nuclei for arbitrary geometries
• Outer jet X-ray and radio emission in R Aquarii: 1999.8 to 2004.0
• Spectral and Timing Nature of the Symbiotic X-ray Binary 4U 1954+319: The Slowest Rotating Neutron Star in an X-ray Binary System
• A new interpretation of the remarkable X-ray spectrum of the symbiotic star CH Cyg
• Observational hints on the torus obscuring gas behaviour through X-rays with NuSTAR data
• An XMM-Newton EPIC X-ray view of the Symbiotic Star R~Aquarii
• Long-term X-ray Variability of the Symbiotic System RT Cru based on Chandra Spectroscopy
• A broadband X-ray study of the asynchronous polar: CD Ind

Cited by in corpus (2)

• Symbiotic stars in the era of modern ground- and space-based surveys
• X-ray Variability in the Symbiotic Binary RT Cru: Principal Component Analysis