Stellar populations in satellite galaxies in close pairs
Satellite galaxies that are near to massive primary galaxies in close pairs can have stellar population ages that are more similar to their primaries than expected. This is one way in which close pairs of galaxies show galactic conformity, which is thought to be driven by assembly bias. Such conformity is seen in ages, morphologies, and star
Sansom, A. E. et al.
Fecha de publicación:
1
2026