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Table 2:

Models successes and failures. The second column shows the successes, while the third column indicates the failures.

Model 
Successes Failures

1
good agreement for the $SFR/SFR_{\odot }$ $\Sigma_{\rm gas}$ not reproduced in the outer Galactic disk
    abundance gradients completely flat
2 good agreement for the $SFR/SFR_{\odot }$ too low $\Sigma_{\rm gas}$ in the inner disk
  increased slope of the gradients in the outer disk abundance gradients too flat in the inner disk
3 good agreement for the $SFR/SFR_{\odot }$ too low $\Sigma_{\rm gas}$
  $\Sigma_{\rm gas}$ increases in the outer part of the disk abundance gradients too flat in the inner disk
  slope of abundance gradients more pronunced in the outer disk  
4 good agreement for the $SFR/SFR_{\odot }$ $\Sigma_{\rm gas}$ not reproduced in the outer Galactic disk
    abundance gradients increase along the galactic disk
5 good agreement for the $SFR/SFR_{\odot }$ $\Sigma_{\rm gas}$ not reproduced in the outer Galactic disk
  slope of abundance gradients more pronunced in the inner disk abundance gradients increase in the outer Galactic disk
6 good agreement for the $SFR/SFR_{\odot }$ $\Sigma_{\rm gas}$ increases along radius
  abundance gradients in good agreement with the observed data  
7 good agreement for the $SFR/SFR_{\odot }$ $\Sigma_{\rm gas}$ too low in the inner part of the Galactic disk
  abundance gradients in good agreement with the observed data  

Source LaTeX | All tables | In the text

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