Massive Star Odyssey

Massive Star Odyssey PDF Author: International Astronomical Union. Scientific Organizing Committee
Publisher:
ISBN:
Category :
Languages : en
Pages :

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Book Description

Massive Star Odyssey

Massive Star Odyssey PDF Author: International Astronomical Union. Scientific Organizing Committee
Publisher:
ISBN:
Category :
Languages : en
Pages :

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Book Description


A Massive Star Odyssey

A Massive Star Odyssey PDF Author: International Astronomical Union. Symposium
Publisher:
ISBN:
Category : Starbursts
Languages : en
Pages : 840

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Book Description


Massive Stars

Massive Stars PDF Author: Space Telescope Science Institute (U.S.). Symposium
Publisher: Cambridge University Press
ISBN: 0521762634
Category : Science
Languages : en
Pages : 253

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Book Description
Presents observational and theoretical papers from world experts addressing the important role in astrophysics of massive stars.

Massive Stars as Cosmic Engines (IAU S250)

Massive Stars as Cosmic Engines (IAU S250) PDF Author: International Astronomical Union. Symposium
Publisher: Cambridge University Press
ISBN: 9780521874724
Category : Science
Languages : en
Pages : 616

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Book Description
Reviews our current understanding of the life, evolution and death of massive stars; for researchers and graduate students.

Star Odyssey

Star Odyssey PDF Author: Jayel Newman
Publisher: AuthorHouse
ISBN: 1463475306
Category : Humor
Languages : en
Pages : 186

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Massive Star Formation

Massive Star Formation PDF Author: Henrik Beuther
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 514

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The Initial Mass Function 50 Years Later

The Initial Mass Function 50 Years Later PDF Author: Edvige Corbelli
Publisher: Springer Science & Business Media
ISBN: 1402034075
Category : Science
Languages : en
Pages : 551

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Book Description
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 Odyssey

Star Odyssey PDF Author: Charles Christian
Publisher:
ISBN: 9781403338914
Category : Fiction
Languages : en
Pages : 320

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Book Description
Mankind has reached the stars, but a warring race from across the galaxy wishes to enslave it, while another seeks all sentient life forms as food--human flesh is its favorite dish. Humanity's true origin then comes into question.

Experimental and Theoretical Advances in Fluid Dynamics

Experimental and Theoretical Advances in Fluid Dynamics PDF Author: Jaime Klapp
Publisher: Springer Science & Business Media
ISBN: 3642179584
Category : Science
Languages : en
Pages : 511

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Book Description
The book is comprised of lectures and selected contributions presented at the Enzo Levi and XVI Annual Meeting of the Fluid Dynamic Division of the Mexican Physical Society in 2010. It is aimed at fourth year undergraduate and graduate students, as well as scientists in the fields of physics, engineering and chemistry with an interest in fluid dynamics from the experimental and theoretical point of view. The lectures are introductory and avoid the use of complicated mathematics. The other selected contributions are also geared to fourth year undergraduate and graduate students. The fluid dynamics applications include multiphase flow, convection, diffusion, heat transfer, rheology, granular material, viscous flow, porous media flow, geophysics and astrophysics. The material contained in the book includes recent advances in experimental and theoretical fluid dynamics and will be of great use to those involved in either teaching and/or research.

Stellar Collapse

Stellar Collapse PDF Author: Chris L. Fryer
Publisher: Springer Science & Business Media
ISBN: 9781402019920
Category : Mathematics
Languages : en
Pages : 454

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Book Description
Supernovae, hypernovae and gamma-ray bursts are among the most energetic explosions in the universe. The light from these outbursts is, for a brief time, comparable to billions of stars and can outshine the host galaxy within which the explosions reside. Most of the heavy elements in the universe are formed within these energetic explosions. Surprisingly enough, the collapse of massive stars is the primary source of not just one, but all three of these explosions. As all of these explosions arise from stellar collapse, to understand one requires an understanding of the others. Stellar Collapse marks the first book to combine discussions of all three phenomena, focusing on the similarities and differences between them. Designed for graduate students and scientists newly entering this field, this book provides a review not only of these explosions, but the detailed physical models used to explain them from the numerical techniques used to model neutrino transport and gamma-ray transport to the detailed nuclear physics behind the evolution of the collapse to the observations that have led to these three classes of explosions.