The galaxy NGC 6503 is not a very bright or massive or big galaxy as they come, however it is relatively isolated in space and thus not expected to have been perturbed by companions. This simplifies studying the gasflow in the galaxy in order to say something sensible about the dark matter contents in a galaxy. Otherwise one could be worried about companions perturbing the dynamics of the gas or stars in this galaxy.
You can clearly see that the immediate neighborhood of NGC 6503 is void of any other galaxies. Most of the visible objects in this picture are stars of our milky way (two are labeled) and a few are fuzzy objects in the far universe catalogues by an Infra Red and Ultra Violet telescope.
See http://cds.u-strasbg.fr/cgi-bin/Dic-Simbad for a service if you ever need to know what that strange astronomy acronym in a source name means...
The following papers discuss this work in more detail:
Searching for non-axisymmetries in NGC 6503: a weak end-on bar (Kuzio de Naray, 2012)
Data on Eric Greisen's website: ftp://ftp.aoc.nrao.edu/staff/egreisen/
We have the following notebooks:
We will not cover:
Related material you can read up on, but not covered here.
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# you could run another notebook here, but it only shows the results.
%run Lecture4-02.ipynb
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