H II Regions and Supernova Remnants
There has been relatively little research done so far on the H II regions of M31, beyond the task of identifying them and cataloging the brightest several hundred. At the time of this writing, however, at least two groups of scientists are working on detailed studies of the H II regions and so this chapter is likely to be outdated to some extent rather soon. For supernova remnants, on the other hand, more has been completed, especially at radio wavelengths.
KeywordsRotation Curve Emission Region Supernova Remnant Luminosity Function Nearby Galaxy
Unable to display preview. Download preview PDF.