On the kinematics of h ii regions: yesterday, today, and tomorrow

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Autor principal: Maite Rozas
Formato: Artículo científico
Lenguaje:en
Publicado: Universidad Nacional Autónoma de México 2002
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author Maite Rozas
author_facet Maite Rozas
contents On the kinematics of h ii regions: yesterday, today, and tomorrow Maite Rozas H. O. Castañeda, Física, Astronomía y Matemáticas HYDRODYNAMICS ISM: H II REGIONS The study of the kinematics and dynamics of H II regions provides us with clues about the physical conditionsof the gas, the interpretation of their emission spectra, and the exchange of mechanical energy between theionizing stars and the ionized gas. We discuss in our presentation the past, present and future research in thiseld. We briey review the theoretical and observational advances performed during the last decades, includingthe study of the e ects of the environment in the kinematics, the champagne model, the supersonic motionsobserved in Giant Extragalactic H II Regions, and the e ects of turbulence and virialization of the gas. Then,we discuss in detail how Fabry-Perot observations, both at single regions and sampling complete galaxies, couldlead us to a better understanding of the physical state of the gas. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112087 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12
format Artículo científico
id redalyc_57112087
institution Redalyc
language en
publishDate 2002
publisher Universidad Nacional Autónoma de México
spellingShingle On the kinematics of h ii regions: yesterday, today, and tomorrow
Maite Rozas
Física, Astronomía y Matemáticas
HYDRODYNAMICS
ISM: H II REGIONS
On the kinematics of h ii regions: yesterday, today, and tomorrow Maite Rozas H. O. Castañeda, Física, Astronomía y Matemáticas HYDRODYNAMICS ISM: H II REGIONS The study of the kinematics and dynamics of H II regions provides us with clues about the physical conditionsof the gas, the interpretation of their emission spectra, and the exchange of mechanical energy between theionizing stars and the ionized gas. We discuss in our presentation the past, present and future research in thiseld. We briey review the theoretical and observational advances performed during the last decades, includingthe study of the e ects of the environment in the kinematics, the champagne model, the supersonic motionsobserved in Giant Extragalactic H II Regions, and the e ects of turbulence and virialization of the gas. Then,we discuss in detail how Fabry-Perot observations, both at single regions and sampling complete galaxies, couldlead us to a better understanding of the physical state of the gas. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112087 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12
title On the kinematics of h ii regions: yesterday, today, and tomorrow
topic Física, Astronomía y Matemáticas
HYDRODYNAMICS
ISM: H II REGIONS
url https://www.redalyc.org/articulo.oa?id=57112087