Astronomy and Astrophysics – Astronomy
Scientific paper
May 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...190.4111d&link_type=abstract
American Astronomical Society, 190th AAS Meeting, #41.11; Bulletin of the American Astronomical Society, Vol. 29, p.834
Astronomy and Astrophysics
Astronomy
Scientific paper
Evidence suggests protostellar collapse can proceed from filamentary or sheet-like cloud cores instead of the spherical cores used in many calculations. We investigate how the collimation of jets or bipolar outflows may be produced by the interaction of a YSO wind with such a filament. Since a collapsing filament forms a toroidal structure, we have specific interest in the effect of the toroid's polar opening angle on the outflow. We present the results of hydrodynamic simulations of the wind-filament interaction, using initial sheet infall conditions from Hartmann, Calvet, and Boss. The simulations are two-dimensional, cylindrically symmetric, and include radiative cooling.
Delamarter Guy
Frank Alejandro
No associations
LandOfFree
Evolution of Outflows In Collapsing Filaments does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Evolution of Outflows In Collapsing Filaments, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of Outflows In Collapsing Filaments will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-831486