Reassessing the Relationship Between Stellar X-ray Luminosity and Age with eROSITA Data Release 1
Nadja Aldarondo Qui\~nones, Sydney Jenkins, Andrew Vanderburg, Melinda Soares-Furtado, Michael A. McDonald

TL;DR
This study reevaluates the correlation between stellar X-ray luminosity and age using eROSITA data, confirming a relationship but highlighting variability and limitations for age estimation accuracy.
Contribution
It provides new X-ray luminosity data for four stars and reassesses the age relationship for 24 older stars, revealing a shallower slope and variability issues.
Findings
Confirmed correlation between X-ray luminosity and age beyond 1 Gyr.
Found a shallower slope in the luminosity-age relationship for older stars.
Identified significant variability in stellar X-ray luminosity affecting age estimates.
Abstract
Accurate stellar dating provides crucial information about the formation and development of planetary systems. Existing age-dating techniques are limited in terms of both the spectral type and age range they can accurately probe, and many are unreliable for stars older than 1 Gyr. Recent studies have suggested that a star's X-ray luminosity correlates strongly with stellar age and shows a steep fall-off at ages older than 1 Gyr. In this work, we present X-ray luminosity relationship values from eROSITA for four previously unassessed stars. Additionally, we reassess the X-ray luminosity/age relationship present in 24 main-sequence stars older than a gigayear. We confirm that a correlation does appear to exist between stellar age and X-ray luminosity at ages older than 1 Gyr. However, we measure a shallower slope with age than previous research for older stars, similar to what was found…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Educational Leadership and Practices
