X-ray activity in pre-main sequence stars

Details X-ray activity in pre-main sequence stars X-ray activity in pre-main sequence stars

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358...75f&link_type=abstract

In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 75-80 (SEE N85-17755 08-88)

Astronomy and Astrophysics

Astronomy

Pre-Main Sequence Stars, Stellar Flares, Stellar Winds, X Rays, Emission Spectra, Line Spectra, X Ray Astronomy

Scientific paper

X-ray findings and their interpretation with respect to winds and surface activity of pre-main sequence stars are summarized. Some recent optical and radio observations supporting the X-ray evidence for giant flares on PMS stars are discussed. The unusual properties of PMS/T Tauri stars were for many years primarily attributed to their strong winds. Numerous lines of evidence are outlined herein indicating that PMS stars also have enhanced surface activity, including extremely strong individual flares.

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