X-ray Emission in Star-Forming Regions

Details X-ray Emission in Star-Forming Regions X-ray Emission in Star-Forming Regions

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cokon.100..369n&link_type=abstract

Communications of the Konkoly Observatory, No. 100 (Vol. XII, 2), p. 369-376 (1997)

Computer Science

Scientific paper

We report on the discovery of hundreds of new T Tauri stars (TTS) in several star forming regions like Taurus-Auriga and Orion. Our target selection for ground-based optical follow-up observations of X-ray sources is based on the large sample of ROSAT All-Sky Survey sources. Most of the newly discovered TTS are weak-line TTS, one of their main characteristics is strong X-ray emission. Based on the spatially complete ROSAT All-Sky Survey, we can confirm that weak-line TTS outnumber classical TTS by a factor between 3 and 10.

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