Name: Qso Absorption Lines: Proceedings of the eso Workshop Held at Garching, Germany, 21–24 November 1994 (Eso Astrophysics Symposia) (en Inglés)
SKU: 62101027
Price: 841.79 MXN
Availability: InStock
Author: Meylan Georges
ISBN: 9783662223734

portada Qso Absorption Lines: Proceedings of the eso Workshop Held at Garching, Germany, 21–24 November 1994 (Eso Astrophysics Symposia) (en Inglés)

Qso Absorption Lines: Proceedings of the eso Workshop Held at Garching, Germany, 21–24 November 1994 (Eso Astrophysics Symposia) (en Inglés)

Formato

Libro Físico

Editorial

Springer

Autor

Meylan Georges

Idioma

Inglés

N° páginas

494

Encuadernación

Tapa Blanda

ISBN13

9783662223734

N° edición

Qso Absorption Lines: Proceedings of the eso Workshop Held at Garching, Germany, 21–24 November 1994 (Eso Astrophysics Symposia) (en Inglés)

Meylan Georges (Autor) · Springer · Tapa Blanda

Libro Nuevo Importado

Envío: 14 a 19 días háb.

$ 1,870.65$ 841.79

-55%

Costos de importación incluídos en el precio ✅

Libro Nuevo

Quedan más de 100 unidades

$ 841.79

¡Envío Gratis! Llega entre el 24 Sep y el 02 Oct a CUAUHTÉMOC, Ciudad de México. Seleccionar ubicación

Agregar a lista de deseos

Reseña del libro "Qso Absorption Lines: Proceedings of the eso Workshop Held at Garching, Germany, 21–24 November 1994 (Eso Astrophysics Symposia) (en Inglés)"

The controversial question of whether the majority of the narrow absorption lines observed in QSO spectra represent cosmological intervening systems or ejecta from the QSO themselves is settled. QSO absorption line spectroscopy, initially a mere technique, has matured into an essential extragalactic research tool for understanding the content of the Universe at redshifts between 0 and 4, and beyond. The only previous important meeting devoted to "QSO Absorption Lines" was held in May 1987 at the Space Telescope Science Institute in Baltimore, Maryland, U.S.A. Since that time, nearly a decade ago, research has been ex- tremely active in this now well-established field of astrophysics. Theoretical stud- ies and simulations have taken advantage of the constant progress in computer technology, and during these last few years, the observational results have bene- fited largely from the new facillities offered by the Hubble Space Telescope in the UV wavelength range and the Keck Telescope for high-resolution spectroscopy.