On the Energetic Component of FU Ori Wind
Observations of short term fluctuations in the Johnson U-band of the star FU Orionis are presented. A preliminary deduction of the flux of the most energetic component of wind particles from such a star is also given.
KeywordsShort Term Fluctuation Photometric Observation Versus Band Tauri Star Flare Event
Unable to display preview. Download preview PDF.
- Pirronello, V., D’Arrigo, C: 1985, “Particle Bombardment of Minor Bodies during Eruptive Phases of the Early Solar Evolution” in “Asteroids, Comet, Meteors”, Lagerkvist C.-I. et al eds., p. 235, Uppsala, Sweden.Google Scholar