Speaker
Federico Lelli
(INAF)
Description
In this talk I will review techniques and idiosyncrasies in building mass models of disk galaxies using cold gas dynamics. I will particularly focus on HI disks, which are generally more extended than stellar disks, so they allow tracing galaxy dynamics out to the most dark-matter-dominated regions. The combination of HI observations and near-infrared photometry, tracing the distribution of stellar mass, has proven extremely powerful to test both LCDM models of galaxy formation and modified gravity theories such as MOND.
Primary author
Federico Lelli
(INAF)