Star Formation, Galaxies and the Interstellar Medium
Star Formation, Galaxies and the Interstellar Medium

Author: Jose Franco

Publisher: Cambridge University Press

Published: 1993-06-10

Total Pages: 418

ISBN-13: 9780521444125

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The enormously powerful phenomena of starbursts are examined in this book. These spectacular star-forming events are seen on large scales in some galaxies, often triggered by galactic interactions. An intriguing implication of starburst research is that active galactic nuclei (AGN) may not be powered by accreting black holes. Instead theories are presented where compact powerhouses of dust-enshrouded star formation lie at the core of AGN, with supernovae exploding roughly once per year within massive nuclear concentrations of gas. This book collects articles from a timely international conference in Elba, Italy, in 1992; these comprise a thorough review of the most important developments in galactic-scale star formation since the starburst revolution of the late 1980s. This text will introduce graduate students to this exciting area and keep experts apace with rapid developments in it.

Introduction to the Interstellar Medium
Introduction to the Interstellar Medium

Author: Jonathan P. Williams

Publisher: Cambridge University Press

Published: 2021-02-18

Total Pages: 221

ISBN-13: 1108480802

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A comprehensive yet accessible textbook introducing the nature of the rarefied matter that pervades the space between stars.

The Formation of Stars
The Formation of Stars

Author: Steven W. Stahler

Publisher: John Wiley & Sons

Published: 2008-07-11

Total Pages: 865

ISBN-13: 3527618686

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This book is a comprehensive treatment of star formation, one of the most active fields of modern astronomy. The reader is guided through the subject in a logically compelling manner. Starting from a general description of stars and interstellar clouds, the authors delineate the earliest phases of stellar evolution. They discuss formation activity not only in the Milky Way, but also in other galaxies, both now and in the remote past. Theory and observation are thoroughly integrated, with the aid of numerous figures and images. In summary, this volume is an invaluable resource, both as a text for physics and astronomy graduate students, and as a reference for professional scientists.

The Interstellar Medium
The Interstellar Medium

Author: James Lequeux

Publisher: Springer Science & Business Media

Published: 2005-08-29

Total Pages: 444

ISBN-13: 3540266933

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Describing interstellar matter in our galaxy in all of its various forms, this book also considers the physical and chemical processes that are occurring within this matter. The first seven chapters present the various components making up the interstellar matter and detail the ways that we are able to study them. The following seven chapters are devoted to the physical, chemical and dynamical processes that control the behaviour of interstellar matter. These include the instabilities and cloud collapse processes that lead to the formation of stars. The last chapter summarizes the transformations that can occur between the different phases of the interstellar medium. Emphasizing methods over results, The Interstellar Medium is written for graduate students, for young astronomers, and also for any researchers who have developed an interest in the interstellar medium.

Physics of the Interstellar and Intergalactic Medium
Physics of the Interstellar and Intergalactic Medium

Author: Bruce T. Draine

Publisher: Princeton University Press

Published: 2010-12-20

Total Pages: 560

ISBN-13: 1400839084

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This is a comprehensive and richly illustrated textbook on the astrophysics of the interstellar and intergalactic medium--the gas and dust, as well as the electromagnetic radiation, cosmic rays, and magnetic and gravitational fields, present between the stars in a galaxy and also between galaxies themselves. Topics include radiative processes across the electromagnetic spectrum; radiative transfer; ionization; heating and cooling; astrochemistry; interstellar dust; fluid dynamics, including ionization fronts and shock waves; cosmic rays; distribution and evolution of the interstellar medium; and star formation. While it is assumed that the reader has a background in undergraduate-level physics, including some prior exposure to atomic and molecular physics, statistical mechanics, and electromagnetism, the first six chapters of the book include a review of the basic physics that is used in later chapters. This graduate-level textbook includes references for further reading, and serves as an invaluable resource for working astrophysicists. Essential textbook on the physics of the interstellar and intergalactic medium Based on a course taught by the author for more than twenty years at Princeton University Covers radiative processes, fluid dynamics, cosmic rays, astrochemistry, interstellar dust, and more Discusses the physical state and distribution of the ionized, atomic, and molecular phases of the interstellar medium Reviews diagnostics using emission and absorption lines Features color illustrations and detailed reference materials in appendices Instructor's manual with problems and solutions (available only to teachers)

The Initial Mass Function 50 Years Later
The Initial Mass Function 50 Years Later

Author: Edvige Corbelli

Publisher: Springer Science & Business Media

Published: 2007-10-06

Total Pages: 551

ISBN-13: 1402034075

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Theideatocelebrate50yearsoftheSalpeterIMFoccurredduringtherecent IAU General Assembly in Sydney, Australia. Indeed, it was from Australia that in July 1954 Ed Salpeter submitted his famous paper "The Luminosity Function and Stellar Evolution" with the rst derivation of the empirical stellar IMF. This contribution was to become one of the most famous astrophysics papers of the last 50 years. Here, Ed Salpeter introduced the terms "original mass function" and "original luminosity function", and estimated the pro- bility for the creation of stars of given mass at a particular time, now known as the "Salpeter Initial Mass Function", or IMF. The paper was written at the Australian National University in Canberra on leave of absence from Cornell University (USA) and was published in 1955 as 7 page note in the Astroph- ical Journal Vol. 121, page 161. To celabrate the 50th anniversary of the IMF, along with Ed Salpeter’s 80th birthday, we have organized a special meeting that brought together scientists involved in the empirical determination of this fundamental quantity in a va- ety of astrophysical contexts and other scientists fascinated by the deep imp- cations of the IMF on star formation theories, on the physical conditions of the gas before and after star formation, and on galactic evolution and cosmology. The meeting took place in one of the most beautiful spots of the Tuscan countryside, far from the noise and haste of everyday life.

Star Formation
Star Formation

Author: Mark R. Krumholz

Publisher: World Scientific Publishing Company

Published: 2017

Total Pages: 507

ISBN-13: 9789813142039

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Observing the cold interstellar medium -- Observing young stars -- Chemistry and thermodynamics -- Gas flows and turbulence -- Magnetic fields and magnetized turbulence -- Gravitational instability and collapse -- Stellar feedback -- Giant molecular clouds escales -- The star formation rate at galactic scales: observations -- The star formation rate at galactic scales: theory -- Stellar clustering -- The initial mass function: observations -- The initial mass function: theory -- Protostellar disks and outflows: observations -- Protostellar disks and outflows: theory -- Protostar formation -- Protostellar evolution -- Massive star formation -- The first stars -- Late-stage stars and disks -- The transition to planet formation

Astrophysics of the Interstellar Medium
Astrophysics of the Interstellar Medium

Author: Giovanni Carraro

Publisher: Springer Nature

Published: 2021-06-22

Total Pages: 356

ISBN-13: 3030752933

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This book is based on a series of lectures for an Astrophysics of the Interstellar Medium (ISM) master’s degree in Astrophysics and Cosmology at Padova University. From the cold molecular phase in which stars and planetary systems form, to the very hot coronal gas that surrounds galaxies and galaxy clusters, the ISM is everywhere. Studying its properties is vital for the exploration of virtually any field in astronomy and cosmology. These notes give the student a coherent and accurate mathematical and physical approach, with continuous references to the real ISM in galaxies. The book is divided into three parts. Part One introduces the equations of fluid dynamics for a system at rest and acoustic waves, and then explores the real ISM through the role of thermal conduction and viscosity, concluding with a discussion of shock waves and turbulence. In Part Two, the electromagnetic field is switched on and its role in modulating shock waves and contrasting gravity is studied. Part Three describes dust and its properties, followed by the main stellar sources of energy. The last two chapters respectively address the various components of the ISM and molecular clouds and star formation.

The Physics of the Interstellar Medium, Second Edition
The Physics of the Interstellar Medium, Second Edition

Author: J.E Dyson

Publisher: CRC Press

Published: 1997-01-01

Total Pages: 184

ISBN-13: 9780585368115

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The book leads the advanced undergraduate through the wide range of disciplines related to an understanding of the interstellar medium and is suitable for any student studying either physics or astrophysics. The study of the interstellar medium incorporates a large range of physical More...processes on both large and small scales all of which are covered in this text. Together with the inclusion of simple models and problems at the end of each chapter this text provides a comprehensive overview and grounding in the study of the interstellar medium.

Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality
Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality

Author: Nickolay Y. Gnedin

Publisher: Springer

Published: 2015-09-09

Total Pages: 375

ISBN-13: 3662478900

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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.