The Factory and the Beehive. IV. A Comprehensive Study of the Rotation X-Ray Activity Relation in Praesepe and the Hyades

Núñez, Alejandro; Agüeros, Marcel A.; Covey, Kevin R.; Douglas, Stephanie T.; Drake, Jeremy J.; Rampalli, Rayna; Bowsher, Emily C.; Cargile, Phillip A.; Kraus, Adam L.; Law, Nicholas M.

doi:10.3847/1538-4357/ac6517

Title: The Factory and the Beehive. IV. A Comprehensive Study of the Rotation X-Ray Activity Relation in Praesepe and the Hyades

Journal Article · Tue May 24 00:00:00 EDT 2022 · The Astrophysical Journal

DOI:https://doi.org/10.3847/1538-4357/ac6517· OSTI ID:1983256

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^[5]; Bowsher, Emily C. ^[1];

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Columbia Univ., New York, NY (United States)
Western Washington University, Bellingham, WA (United States)
Lafayette College, Easton, PA (United States)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Dartmouth College, Hanover, NH (United States)
Univ. of Texas, Austin, TX (United States)
Univ. of North Carolina, Chapel Hill, NC (United States)

X-ray observations of low-mass stars in open clusters are critical to understanding the dependence of magnetic activity on stellar properties and their evolution. Praesepe and the Hyades, two of the nearest, most-studied open clusters, are among the best available laboratories for examining the dependence of magnetic activity on rotation for stars with masses ≲1 M_⊙. We present an updated study of the rotation–X-ray activity relation in the two clusters. We updated membership catalogs that combine pre-Gaia catalogs with new catalogs based on Gaia Data Release 2. The resulting catalogs are the most inclusive ones for both clusters: 1739 Praesepe and 1315 Hyades stars. We collected X-ray detections for cluster members, for which we analyzed, re-analyzed, or collated data from ROSAT, the Chandra X-ray Observatory, the Neil Gehrels Swift Observatory, and XMM-Newton. We have detections for 326 Praesepe and 462 Hyades members, of which 273 and 164, respectively, have rotation periods—an increase of 6× relative to what was previously available. We find that at ≈700 Myr, only M dwarfs remain saturated in X-rays, with only tentative evidence for supersaturation. We also find a tight relation between the Rossby number and fractional X-ray luminosity L_X/L_bol in unsaturated single members, suggesting a power-law index between –3.2 and –3.9. Lastly, we find no difference in the coronal parameters between binary and single members. These results provide essential insight into the relative efficiency of magnetic heating of the stars' atmospheres, thereby informing the development of robust age-rotation-activity relations.

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Research Organization:: US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)

Sponsoring Organization:: USDOE Office of Science (SC); National Science Foundation (NSF); National Aeronautics and Space Administration (NASA); Alfred P. Sloan Foundation

Grant/Contract Number:: 2138089; NNX17AD71G; NAS8-39073

OSTI ID:: 1983256

Journal Information:: The Astrophysical Journal, Vol. 931, Issue 1; ISSN 0004-637X

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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