Star Formation, 1st ed. 2021 Space Sciences Series of ISSI Series, Vol. 83
Coordonnateurs : Bykov Andrei M., Charbonnel Corinne, Hennebelle Patrick, Marcowith Alexandre, Meynet Georges, Falanga Maurizio, von Steiger Rudolf
- The role of gravity and magnetized turbulence in the formation and evolution of molecular clouds
- The stellar feedback (supernovae, HII regions, winds, cosmic rays) in regulating star formation
- The origin of the stellar initial mass function and its universality across various environments
- Jets, magnetic fields and high energy particles in stellar clusters
- The origin of the first stars and black holes
Editorial.- Physical processes in Star Formation.- The molecular cloud lifecycle.- From diffuse gas to dense molecular cloud cores.- The origin of the stellar mass distribution and multiplicity.- Zooming in on Individual Star Formation: Low- and High-mass Stars.- Star clusters near and far; tracing star formation across cosmic time.- The Physics of Star Cluster Formation and Evolution.- Formation and Evolution of Disks around Young Stellar Objects.- Formation of the first stars and black holes.- Impact of low-energy cosmic rays on star formation.- High-energy particles and radiation in star-forming regions.
Corinne Charbonnel is professor of Astrophysics at the University of Geneva (Switzerland) and Senior Researcher at CNRS (France). She was the President of the French Society of Astronomy and Astrophysics (SF2A) and of Division G (Stars and Stellar Physics) of the International Astronomical Union (IAU). She has pioneered studies of the impact of magnetohydrodynamical mechanisms on the transport of angular momentum and of chemicals in stellar interiors. She studies the broad consequences of these processes on stellar evolution and nucleosynthesis, planet habitability, stellar population properties across cosmic time, and the chemical and dynamical evolution of star clusters and galaxies.
Patrick Hennebelle is an expert of the star formation process and the dynamics of the interstellar medium. He performs heavy numerical simulations that he confronts on one hand to analytical models and on the other hand to observations. He has particularly been working on the formation of molecular clouds, the collapse of dense cores, the formation of planet-forming discs and the origin of the stellar initial mass function.
Alexandre Marcowith is staff researcher in the high-energy astrophysics department at Montpellier university. His research is centred on the physics and Astrophysics of Cosmic Rays focusing on acceleration and transport processes in the inter-stellar medium. He is member of the High Energy Stereoscopic System
Provides a unique, multidisciplinary review of star formation in astrophysics
Written by globally recognized experts actively working in the field
Useful for specialists and early career researchers
Date de parution : 10-2021
Ouvrage de 553 p.
15.5x23.5 cm
Date de parution : 10-2020
Ouvrage de 553 p.
15.5x23.5 cm