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2007MNRAS.379L..35G - Mon. Not. R. Astron. Soc., 379, L35-L39 (2007/July-3)
Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors ?
GREGORY S.G., WOOD K. and JARDINE M.
Abstract (from CDS):
Abstract Copyright: 2007 The Authors. Journal compilation © 2007 RAS
Journal keyword(s): stars: activity - stars: coronae - stars: magnetic fields - stars: pre-main-sequence - X-rays: stars
Simbad objects: 7
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