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The warm ionized medium in spiral galaxies

Bibcode
2009RvMP...81..969H
DOI
10.1103/RevModPhys.81.969
Haffner, L. M.; Dettmar, R.-J.; Beckman, J. E.; Wood, K.; Slavin, J. D.; Giammanco, C.; Madsen, G. J.; Zurita, A.; Reynolds, R. J.
Referencia bibliográfica

Reviews of Modern Physics, vol. 81, Issue 3, pp. 969-997

Fecha de publicación:
7
2009
Revista
Reviews of Modern Physics
Número de autores
9
Número de autores del IAC
2
Número de citas
292
Número de citas referidas
259
Descripción
This article reviews observations and models of the diffuse ionized gas that permeates the disk and halo of our Galaxy and others. It was inspired by a series of invited talks presented during an afternoon scientific session of the 65th birthday celebration for Professor Carl Heiles held at Arecibo Observatory in August 2004. This review is in recognition of Carl’s long-standing interest in and advocacy for studies of the ionized as well as the neutral components of the interstellar medium.
Proyectos relacionados
Poster Almeria Astronomy week
Estudios Cinemáticos, Estructurales y de Composición, de los Medios Interestelares e Intergalácticos
El objetivo básico del proyecto es investigar la evolución de las galaxias mediante el entendimiento de la interacción del medio interestelar y las estrellas. La técnica principal que utilizamos es la cinemática bidimensional de galaxias enteras observada por nuestro instrumento GHaFaS, un interferometro Fabry Perot en el telescopio William
Prof.
John E. Beckman
En ejecución
Tipo
Con árbitro
Formación y Evolución de Galaxias (FYEG)

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