Mechanical energy release by protostars to molecular clouds

Details Mechanical energy release by protostars to molecular clouds Mechanical energy release by protostars to molecular clouds

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.207..235s&link_type=abstract

In ESA Plasma Astrophys. p 235-236 (SEE N85-22270 12-90)

Astronomy and Astrophysics

Astrophysics

Molecular Clouds, Stellar Mass Ejection, T Tauri Stars, Astronomical Models, Herbig-Haro Objects, Stellar Winds

Scientific paper

Outburst activity of low mass stars embedded in molecular clouds is proposed as a source of energy at least comparable to winds from massive stars and protostars. Low-mass stars appear to have more intense activity than previously thought. They are more numerous and more evenly distributed within the cloud, and could play the main role in providing pressure support to the system.

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