Name: Spectroscopy: The key to the Stars: Reading the Lines in Stellar Spectra (The Patrick Moore Practical Astronomy Series) (en Inglés)
Price: 44770.00 CLP
Availability: InStock
Author: Robinson, Keith
ISBN: 9780387367866

portada Spectroscopy: The key to the Stars: Reading the Lines in Stellar Spectra (The Patrick Moore Practical Astronomy Series) (en Inglés)

Formato

Libro Físico

Autor

Keith Robinson

Editorial

Springer

Año

2007

Idioma

Inglés

N° páginas

160

Encuadernación

Tapa Blanda

Dimensiones

23.4 x 15.7 x 0.9 cm

Peso

0.30 kg.

ISBN

0387367861

ISBN13

9780387367866

N° edición

2007

Categorías

Astronomía, espacio y tiempo

Spectroscopy: The key to the Stars: Reading the Lines in Stellar Spectra (The Patrick Moore Practical Astronomy Series) (en Inglés)

Keith Robinson (Autor) · Springer · Tapa Blanda

Libro Nuevo

$ 44.770

$ 74.610

Ahorras: $ 29.840

40% descuento

Envío normal

Origen: Estados Unidos (Costos de importación incluídos en el precio)

Se enviará desde nuestra bodega entre el Martes 14 de Mayo y el Jueves 23 de Mayo.

Lo recibirás en cualquier lugar de Chile entre 1 y 3 días hábiles luego del envío.

Reseña del libro "Spectroscopy: The key to the Stars: Reading the Lines in Stellar Spectra (The Patrick Moore Practical Astronomy Series) (en Inglés)"

Most amateur astronomers may know about red shift, and have a general idea of the ways that stellar spectra provide insight into the atomic processes of the star, but detailed knowledge is unusual. This is because most available books are pitched at professional astronomers and college-level students, and are difficult to read. This is the first non-technical book on spectroscopy, written specifically for practical amateur astronomers. It includes all the science needed for a qualitative understanding of stellar spectra, but avoids bogging down in heavy math. It's the only book written for the amateur astronomer interested in and doing observational spectroscopy, who wants a non-technical account of the physical processes that determine the intensity and profile morphology of lines in stellar spectra. Of course, "armchair astronomers" who simply want to understand the physical processes which shape lines in stellar spectra will find this book equally fascinating.