SIMBAD references

1995A&A...295..335C - Astronomy and Astrophysics, volume 295, 335-346 (1995/3-2)

A generalized Schmidt star formation law: observational constraints.

CAIMMI R.

Abstract (from CDS):

This paper aims to see whether a generalized Schmidt star formation law is consistent with observations in the light of a closed, comoving model of chemical evolution, where two main phases occurred: contraction (extended component) and equilibrium (flat component). It is shown that the empirical relation between present-day gas mass which is being turned into stars and gas mass, {dot}(M)ga∝Mga, i.e. a linear correlation between the model present-day star formation rate and gas mass fraction, CD∝µa, yields a connection between the ratio of contraction time to age, Tc/T, and µa. The comparison between model predictions and observations leads to the following main conclusions: (i) models where star formation obeys a pure Schmidt law cannot fit the whole set of observations; (ii) if we demand (in dealing with an averaged CDa)Tc/T>0 for all the galaxies and Tc/T<0.5 for at least a fraction of large-mass (M>1011M) galaxies of the sample considered, then a generalized Schmidt star formation law with an exponent n≃1 is preferred in respect to n≃2; (iii) if contraction and equilibrium phase were characterized by different star formation rates and mass spectra, then a correlation exists between present-day metal content and gas mass fraction. Thus a generalized Schmidt star formation law with exponent n≃1 appears to be consistent with observations.

Abstract Copyright:

Journal keyword(s): galaxies: evolution - abundances - stars: formation - evolution

Simbad objects: 72

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:1995A&A...295..335C and select 'bookmark this link' or equivalent in the popup menu


2020.08.13-02:59:34

© Université de Strasbourg/CNRS

    • Contact