Stellar feedback and the energy budget of late-type Galaxies: missing baryons and core creation
In a ΛCDM cosmology, galaxy formation is a globally inefficient process: it is often the case that far fewer baryons are observed in galaxy discs than expected from the cosmic baryon fraction. The location of these `missing baryons' is unclear. By fitting halo profiles to the rotation curves of galaxies in the SPARC data set, we measure the
Katz, H. et al.
Fecha de publicación:
11
2018