Name: the physics of star formation and early stellar evolution (en Inglés)
SKU: 3404851
Price: 104.94 USD
Availability: InStock
Author: Lada, Charles J. ; Kylafis, N. D.
ISBN: 9780792313670

portada the physics of star formation and early stellar evolution (en Inglés)

the physics of star formation and early stellar evolution (en Inglés)

Formato

Libro Físico

Ilustrado por

Charles J. Lada

N. D. Kylafis

Editorial

Springer

Autor

Lada, Charles J. ; Kylafis, N. D.

Idioma

Inglés

N° páginas

780

Encuadernación

Tapa Blanda

Dimensiones

23.4x15.6x4 cm

Peso

1.08 kg.

ISBN

0792313674

ISBN13

9780792313670

Categorías

Astronomía, espacio y tiempo
Astrofísica

the physics of star formation and early stellar evolution (en Inglés)

Charles J. Lada (Ilustrado por) · N. D. Kylafis (Ilustrado por) · Springer · Tapa Blanda

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Reseña del libro "the physics of star formation and early stellar evolution (en Inglés)"

The origin of stars is one of the principle mysteries of nature. During the last two decades advances in technology have enabled more progress to be made in the quest to understand stellar origins than at any other time in history. The study of star formation has developed into one of the most important branches of mod- ern astrophysical research. A large body of observational data and a considerable literat ure now exist concerning this topic and a 1arge community of international astronomers and physicists devote their efforts attempting to decipher the secrets of stellar birth. Yet, the young astronomerjphysicist or more advanced researcher desiring to obtain a basic background in this area of research must sift through a very diverse and sometimes bewildering literature. A literature which includes research in many discip1ines and sub discip1ines of classical astrophysics from stel- lar structure to the interstellar medium and encompasses the entire range of the electromagnetic spectrum from radio to gamma rays. Often, the reward of a suc- cessfu1 foray through the current literature is the realization that the results can be obsolete and outdated as soon as the ink is dry in the journal or the conference proceeding in which they are published.