An XMM-Newton EPIC X-Ray View of the Symbiotic Star R Aquarii

• Published in: Astrophysical journal. Letters Vol. 927; no. 1; p. L20
• Main Authors: Toalá, Jesús A., Sabin, Laurence, Guerrero, Martín A., Ramos-Larios, Gerardo, Chu, You-Hua
• Format: Journal Article
• Language: English
• Published: Austin The American Astronomical Society 01.03.2022; IOP Publishing
• Subjects: Accretion disks; Active galaxies; Clumps; Emission analysis; Galaxies; Low mass stars; Magnetic fields; Nebulae; Soft x rays; Spatial distribution; Stellar jets; Stellar winds; Symbiotic binary stars; Symbiotic stars; X ray imagery; X-ray astronomy; X-ray emissions; X-ray sources; X-rays; XMM (spacecraft)
• ISSN: 2041-8205; 2041-8213
• DOI: 10.3847/2041-8213/ac589d

Abstract We present the analysis of archival XMM-Newton European Photon Imaging Camera (EPIC) X-ray observations of the symbiotic star R Aquarii. We used the Extended Source Analysis Software package to disclose diffuse soft X-ray emission extending up to 2.′2 (≈0.27 pc) from this binary system. The depth of these XMM-Newton EPIC observations reveals in unprecedented detail the spatial distribution of this diffuse emission, with a bipolar morphology spatially correlated with the optical nebula. The extended X-ray emission shares the same dominant soft X-ray-emitting temperature as the clumps in the jet-like feature resolved by Chandra in the vicinity of the binary system. The harder component in the jet might suggest that the gas cools down; however, the possible presence of nonthermal emission produced by the presence of a magnetic field collimating the mass ejection cannot be discarded. We propose that the ongoing precessing jet creates bipolar cavities filled with X-ray-emitting hot gas that feeds the more extended X-ray bubble as they get disrupted. These EPIC observations demonstrate that the jet feedback mechanism produced by an accreting disk around an evolved, low-mass star can blow hot bubbles, similar to those produced by jets arising from the nuclei of active galaxies.