in galaxies
Diapositiva 1
Diapositiva 1
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c(Hβ)<br />
Redden<strong>in</strong>g<br />
-Quotients of the detected Balmer l<strong>in</strong>es (Hα, Hβ, Hγ and Hδ)<br />
and Hβ <strong>in</strong> relation to the theoretical expected values and the<br />
ext<strong>in</strong>ction curve.<br />
-Slope estimator constant of redden<strong>in</strong>g<br />
-Galactic ext<strong>in</strong>ction is negligible<br />
-Only knots well covered by the slit lead to values of C(Hβ)<br />
clearly larger than 0.
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