Lavoisier S.A.S.
14 rue de Provigny
94236 Cachan cedex
FRANCE

Heures d'ouverture 08h30-12h30/13h30-17h30
Tél.: +33 (0)1 47 40 67 00
Fax: +33 (0)1 47 40 67 02


Url canonique : www.lavoisier.fr/livre/astronomie/star-formation/descriptif_4418934
Url courte ou permalien : www.lavoisier.fr/livre/notice.asp?ouvrage=4418934

Star Formation, 1st ed. 2021 Space Sciences Series of ISSI Series, Vol. 83

Langue : Anglais

Coordonnateurs : Bykov Andrei M., Charbonnel Corinne, Hennebelle Patrick, Marcowith Alexandre, Meynet Georges, Falanga Maurizio, von Steiger Rudolf

Couverture de l’ouvrage Star Formation
The review papers in this volume provide an in-depth examination of complex astrophysical phenomena of star formation via multi-wavelength observations and modeling. 
Among the fundamental issues discussed in the book are: 
  • 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
The goal of these papers is to review the major processes governing star formation and to investigate how they are interlinked. In doing so, they provide an in-depth look at the tremendous theoretical and observational progress that has been made in the recent past and also outline future perspectives.

Previously published in Space Science Reviews in the Topical Collection "Star Formation?

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.

Andrei Bykov is head of High Energy Astrophysics laboratory in the Ioffe Institute, corresponding member of the Russian Academy of Sciences. His principal research interests are theory and observations of processes in astrophysical objects with extreme energy release ‐ supernovae, gamma‐ray bursts and clusters of galaxies. He is author and coauthor of over 250 scientific publications, a book on Turbulence, Current Sheets and Shocks in Cosmic Plasmas and editor of seven books on high energy astrophysics.

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 :

Ouvrage de 553 p.

15.5x23.5 cm

Disponible chez l'éditeur (délai d'approvisionnement : 15 jours).

137,14 €

Ajouter au panier

Date de parution :

Ouvrage de 553 p.

15.5x23.5 cm

Disponible chez l'éditeur (délai d'approvisionnement : 15 jours).

137,14 €

Ajouter au panier