X-Rays from the Youngest Stars in the Corona Australis Cloud

Details X-Rays from the Youngest Stars in the Corona Australis Cloud X-Rays from the Youngest Stars in the Corona Australis Cloud

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..218g&link_type=abstract

Chandra Proposal ID #01200043

Physics

Chandra Proposal Id #01200043

Scientific paper

Low-mass pre-main sequence stars from protostars to post-T Tauri stars have X-ray emission considerably above that seen in older stars. Powerful flares from Class I protostars are particularly important and poorly understood. The core of the nearby star forming cloud in Corona Australis contains several X-ray emitting protostars as well as T Tauri and Herbig Ae/Be stars with associated outflows.

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