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

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arxiv 2401.17273 v1 pith:UEIWH677 submitted 2024-01-30 astro-ph.SR astro-ph.GA

classification astro-ph.SRastro-ph.GA
keywords x-raysamplecatalogerositastarsall-skyemissionentries
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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.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The stellar corona-chromosphere connection. A comprehensive study of X-ray and Ca II IRT fluxes from eROSITA and Gaia

    astro-ph.SR 2025-04 conditional novelty 7.0 of 10

    X-ray and Ca II infrared triplet activity in 43,200 late-type stars correlate tightly for active stars, saturate together near a Rossby number of about -1.4, and show a gradual flux-flux relation instead of two branches.

  2. Cataclysmic variables from SRG/eROSITA: new systems from eRASS1

    astro-ph.SR 2026-07 accept novelty 6.0 of 10

    A Random Forest plus Gaia/eROSITA match yields 156 spectroscopically confirmed CVs from eRASS1, spanning subtypes, periods, and luminosities, with the method outperforming several published alternatives.

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