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Evolution of X-Ray Activity in <25 Myr Old Pre-main Sequence Stars
Konstantin V. Getman et al 2022 The Astrophysical Journal 935 .
Caption: Figure 3.
Gaia astrometry of X-Ray and non-X-Ray sources toward NGC 869 = h Per. See Figure 2 caption for explanation.
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© 2022. The Author(s). Published by the American Astronomical Society.
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