On star formation rate and turbulent dissipation in galactic models

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dc.creatorKurbatov, E. P.
dc.date2007-05-18
dc.date2007-12-10
dc.date.accessioned2026-07-07T08:47:50Z
dc.date.available2026-07-07T08:47:50Z
dc.descriptionThe 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.
dc.descriptionPublished in Proceedings of the 14th Young Scientists Conference on Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007
dc.identifierhttps://arxiv.org/abs/0705.2653
dc.identifierhttp://arxiv.org/abs/0705.2653
dc.identifierYSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A. Golovin), Kyiv, Kyivskyi Universytet, pp. 54-58, 2007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143739
dc.subjectAstrophysics
dc.titleOn star formation rate and turbulent dissipation in galactic models
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