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2002ApJ...567..434K - Astrophys. J., 567, 434-440 (2002/March-1)
Evidence for accretion: high-resolution X-ray spectroscopy of the classical T Tauri star TW Hydrae.
KASTNER J.H., HUENEMOERDER D.P., SCHULZ N.S., CANIZARES C.R. and WEINTRAUB D.A.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Circumstellar Matter - Stars: Formation - Stars: Individual: Constellation Name: TW Hydrae - X-Rays: Stars
Simbad objects: 11
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