''Forbidden" stars in the eROSITA all-sky survey: X-ray emission from very late-type giants

• Published in: arXiv.org 2024-01
• Main Authors: J H M M Schmitt, Hünsch, M, Schneider, P C, Freund, S, Czesla, S, Robrade, J, Schwope, A
• Format: Article
• Language: English
• Subjects: Data analysis; Emission analysis; Sky surveys (astronomy); Supergiant stars; X ray sources; X ray spectra; X-ray astronomy; XMM (spacecraft)
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2401.17273

We present the results of the first X-ray all-sky survey (eRASS1) performed by the eROSITA instrument onboard the Spectrum-Roentgen-Gamma (SRG) mission on X-ray emitting red giants and supergiants. Focussing on stars positioned at high galactic latitudes above 20 deg, we construct a complete sample of such objects using the Gaia DR3 catalog and identify a sample 96 stars appearing as bona fide entries in the eRASS1 source catalog. Restricting again the sample to objects nearer than 1300~pc and eliminating all catalog entries which are due to optical contamination, we end up with a sample of 16 genuine red giant/supergiant X-ray sources, which represent -- with the exception of one source (CL~Hyi) -- new X-ray detections. We furthermore present a low SNR X-ray spectrum of the nearby low activity giant Arcturus obtained from a pointed observation with the XMM-Newton satellite and give a detailed account of our data analysis. We show that Arcturus-like X-ray emission cannot be the explanation for the X-ray emissions observed by eROSITA and provide a discussion of the possible nature of the detected X-ray sources.