X-ray and optical studies of low-mass star formation.

Details X-ray and optical studies of low-mass star formation. X-ray and optical studies of low-mass star formation.

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994xosl.book.....a&link_type=abstract

X-ray and optical studies of low-mass star formation., by Alcalá-Estrada, J. M.. Heidelberg Univ. (Germany). Naturwissenschaftli

Physics

Scientific paper

Weak-line T Tauri stars (WTTS) are low-mass pre-main sequence stars which lack both the strong emission lines and IR excesses typical of classical T Tauri stars. Most of them have been discovered on the basis of their solar-like X-ray emission. In this work, X-ray data from the ROSAT all-sky survey in the Chamaeleon and the Orion star forming regions, and from one ROSAT pointed observation in the Cha I dark cloud, were used to determine the number of WTTS, to investigate their spatial distribution, and to study their physical properties and their X-ray emission.

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