TW Hya: Spectral variability, X-rays, and accretion diagnostics

The nearest accreting T Tauri star, TW Hya was intensively and continuously observed over ∼17days with spectroscopic and photometric measurements from four continents simultaneous with a long segmented exposure using the Chandra satellite. Contemporaneous optical photometry from WASP-S indicates a 4...

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Detalles Bibliográficos
Autores principales:	Dupree, A.K., Brickhouse, N.S., Cranmer, S.R., Luna, G.J.M., Schneider, E.E., Bessell, M.S., Bonanos, A., Crause, L.A., Lawson, W.A., Mallik, S.V., Schuler, S.C.
Formato:	JOUR
Materias:	accretion, accretion disks stars: individual (TW Hydrae) stars: pre-main sequence stars: variables: T Tauri, Herbig Ae/Be stars: winds, outflows
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v750_n1_p_Dupree
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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