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The Interaction of Fast Particles with Frozen Gases in T Tau Nebulae: The Physical Background

Published online by Cambridge University Press:  12 April 2016

V. Pirronello
Affiliation:
Istituto di Fisica, Facoltà di Ingegneria, Catania, Italy Osservatorio Astrofisico di Catania, Italy
G. Strazzulla
Affiliation:
Osservatorio Astrofisico di Catania, Italy
G. Foti
Affiliation:
Istituto di Struttura della Materia, Università di Catania

Extract

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The interaction of energetic particles with frozen gas layers plays a relevant role in a variety of astrophysical scenarii and also in T Tau nebulae because of the large fluxes of particles ejected by these stars during their continuous flaring activity and the observed presence of ice grains at least around the very young star KL Tau (Cohen, 1975).

Type
Session III: Observed Activity in Related Objects
Copyright
Copyright © Reidel 1983

References

REFERENCES

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Ciavola, G., Foti, G., Torrisi, L., Pirronello, V., Strazzulla, G.: 1982, Radiation Effects (in press).Google Scholar
Cohen, M.: 1975, M.N.R.A.S. 173, 279.Google Scholar
Pirronello, V., Strazzulla, G., Foti, G., Rimini, E.: 1981, Astron. Astrophys. 96, 267.Google Scholar