the University of Oregon Physics Department
Here students will have an opportunity to measure redshifts for several galaxies using a set of common spectral lines here. While the spectra that students will be using have many lines (emission and absorption) students must concentrate on using the following sets: calcium H and K and hydrogen emission lines . Students are asked to determine if there is a correlation between the presence of emission lines in the spectra and the overall appearance (morphology) of the galaxy.
%0 Electronic Source %A University of Oregon Physics Department, %T The Hubble Law %V 2018 %N 19 March 2018 %9 application/java %U http://zebu.uoregon.edu/nsf/hub.html
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