THICK DISCS AND TRUNCATIONS IN SPIRAL GALAXIES
Our understanding of the evolution of galaxies within their optical radius has made great advances in the last decades. These have been achieved by analysing in detail the internal secular processes, the star formation history, and the Interstellar medium. However, the study of galaxy outskirts, so-called low surface brightness science, is still in
Cristina Martínez Lombilla
Fecha de publicación:
4
2018