On star formation rate and turbulent dissipation in galactic models

Details On star formation rate and turbulent dissipation in galactic models On star formation rate and turbulent dissipation in galactic models

2007-05-18

arxiv.org/abs/0705.2653v4

YSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A. Golovin), Kyiv, Kyivskyi Universytet, pp. 54-58, 2007

Astronomy and Astrophysics

Astrophysics

Published in Proceedings of the 14th Young Scientists Conference on Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2

Scientific paper

The models of star formation function and of dissipation of turbulent energy
of interstellar medium are proposed. In star formation model the feedback of
supernovae is taken into account. It is shown that hierarchical scenario of
galaxy formation with proposed models is able to explain the observable star
formation pause in the Galaxy.

Affiliated with

Also associated with

No associations

Rating

On star formation rate and turbulent dissipation in galactic models 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 On star formation rate and turbulent dissipation in galactic models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On star formation rate and turbulent dissipation in galactic models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-438677