Book contents
- Frontmatter
- Contents
- List of Figures
- List of Tables
- List of Contributors
- Preface
- Part I Background
- 1 Introduction
- 2 The Initial Mass Function of Stars and the Star-Formation Rates of Galaxies
- 3 Stellar Populations, Stellar Evolution, and Stellar Atmospheres
- 4 Dust Extinction, Attenuation, and Emission
- Part II SFR Measurements
- Index
1 - Introduction
from Part I - Background
Published online by Cambridge University Press: 11 May 2021
- Frontmatter
- Contents
- List of Figures
- List of Tables
- List of Contributors
- Preface
- Part I Background
- 1 Introduction
- 2 The Initial Mass Function of Stars and the Star-Formation Rates of Galaxies
- 3 Stellar Populations, Stellar Evolution, and Stellar Atmospheres
- 4 Dust Extinction, Attenuation, and Emission
- Part II SFR Measurements
- Index
Summary
Stars play such a fundamental role in the evolution of galaxies, some of the key-questions in the field of galaxy evolution and cosmology are related to the history of their formation in galaxies. How do star formation and its history depend on the environment or on the mass of galaxies? When do stars form globally in the history of the universe ? When and how does starlight contribute to the re-ionization phase in the early universe?The goal of this book is to provide the reader an overall presentation of the theoretical and observational backgrounds about the definition and measurement of Star-Formation Rates in galaxies
- Type
- Chapter
- Information
- Star-Formation Rates of Galaxies , pp. 3 - 24Publisher: Cambridge University PressPrint publication year: 2021