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Star formation in galaxy evolution connecting numerical models to reality : Saas-Fee Advanced course 43 /
This book contains the elaborated and updated versions of the 24 lectures given at the 43rd Saas-Fee Advanced Course. Written by four eminent scientists in the field, the book reviews the physical processes related to star formation, starting from cosmological down to galactic scales. It presents a...
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Main Authors: | , , , |
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Other Authors: | , , , |
Format: | eBook |
Language: | English |
Published: |
Heidelberg :
Springer,
[2015]
|
Series: | Saas-Fee advanced course ... lecture notes ;
43. |
Physical Description: |
1 online resource (xi, 365 pages) : illustrations (some color). |
Subjects: |
Stars
-- Formation.
|
Online Access: | SpringerLink - Click here for access |
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245 | 0 | 0 | |a Star formation in galaxy evolution : |b connecting numerical models to reality : Saas-Fee Advanced course 43 / |c Swiss Society for Astrophysics and Astronomy ; Nickolay Y. Gnedin, Simon C.O. Glover, Ralf S. Klessen, Volker Springel ; edited by Yves Revaz, Pascale Jablonka, Romain Teyssier, Lucio Mayer. |
264 | 1 | |a Heidelberg : |b Springer, |c [2015] | |
264 | 4 | |c ©2016. | |
300 | |a 1 online resource (xi, 365 pages) : |b illustrations (some color). | ||
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490 | 1 | |a Saas-Fee Advanced Course, |x 1861-7980 ; |v 43. | |
504 | |a Includes bibliographical references and index. | ||
588 | 0 | |a Online resource; title from PDF title page (SpringerLink, viewed September 17, 2015). | |
520 | |a This book contains the elaborated and updated versions of the 24 lectures given at the 43rd Saas-Fee Advanced Course. Written by four eminent scientists in the field, the book reviews the physical processes related to star formation, starting from cosmological down to galactic scales. It presents a detailed description of the interstellar medium and its link with the star formation. And it describes the main numerical computational techniques designed to solve the equations governing self-gravitating fluids used for modelling of galactic and extra-galactic systems. This book provides a unique framework which is needed to develop and improve the simulation techniques designed for understanding the formation and evolution of galaxies. Presented in an accessible manner it contains the present day state of knowledge of the field. It serves as an entry point and key reference to students and researchers in astronomy, cosmology, and physics. | ||
505 | 0 | |a Physical Processes in the Interstellar Medium -- High performance computing and numerical modelling -- Index. | |
650 | 0 | |a Stars |x Formation. |0 https://id.loc.gov/authorities/subjects/sh85127431. | |
650 | 0 | |a Galaxies |x Evolution. |0 https://id.loc.gov/authorities/subjects/sh85052765. | |
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650 | 6 | |a Galaxies |x Évolution. | |
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650 | 7 | |a Stars |x Formation. |2 fast. | |
700 | 1 | |a Gnedin, Nickolay Y., |d 1966- |0 https://id.loc.gov/authorities/names/nr94031555 |1 https://id.oclc.org/worldcat/entity/E39PCjwx8RBrd9Xjgty64WwyFq, |e author. | |
700 | 1 | |a Glover, Simon C. O., |e author. | |
700 | 1 | |a Klessen, Ralf S., |0 https://id.loc.gov/authorities/names/nb2015001660 |e author. | |
700 | 1 | |a Springel, Volker, |e author. | |
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700 | 1 | |a Jablonka, Pascale, |0 https://id.loc.gov/authorities/names/nb2016020716 |e editor. | |
700 | 1 | |a Teyssier, Romain, |e editor. | |
700 | 1 | |a Mayer, Lucio, |0 https://id.loc.gov/authorities/names/no2021011796 |e editor. | |
710 | 2 | |a Schweizerische Gesellschaft für Astrophysik und Astronomie, |0 https://id.loc.gov/authorities/names/n50054473 |e sponsoring body. | |
776 | 0 | 8 | |i Print version: |t Star formation in galaxy evolution. |d Heidelberg : Springer, [2015] |z 3662478897 |z 9783662478899 |w (OCoLC)911210661. |
830 | 0 | |a Saas-Fee advanced course ... lecture notes ; |0 https://id.loc.gov/authorities/names/n91076152 |v 43. | |
880 | 0 | |6 505-00/(S |a Preface; Contents; Modeling Physical Processes at Galactic Scales and Above; 1 In Lieu of Introduction; 2 Physics of the IGM; 2.1 Linear Hydrodynamics in the Expanding Universe; 2.2 Lyman-α Forest; 2.3 Modeling the IGM; 2.4 What Observations Tell Us; 3 From IGM to CGM; 3.1 Large Scale Structure; 3.2 How Gas Gets onto Galaxies; 3.3 Cool Streams; 3.4 Galactic Halos; 3.5 Diversion: Cooling of Rarefied Gases; 3.6 Back to Galactic Halos; 4 ISM: Gas in Galaxies; 4.1 Galaxy Formation Lite; 4.2 Galactic Disks; 4.3 Ionized, Atomic, and Molecular Gas in Galaxies; 4.4 Molecular ISM; 5 Star Formation. | |
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