Some theoretical consequences of the thick, magnetized galactic disk
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| Formato: | Artículo científico |
| Lenguaje: | en |
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Universidad Nacional Autónoma de México
2001
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| _version_ | 1876466694007816192 |
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| author | Marco A. Martos |
| author_facet | Marco A. Martos |
| contents | Some theoretical consequences of the thick, magnetized galactic disk Marco A. Martos Física, Astronomía y Matemáticas MHD GALAXY: HALO GALACTIC: STRUCTURE A number of recent observational studies reveal a new paradigm for diskgalaxies, one in which layers of warm ionized gas, dust structures and magneticelds commonly extend to considerable heights (of kpc) above their midplanes.This thick disk has an intricate and largely unknown structure. Its inclusion whilemodeling large scale dynamical processes in the interstellar medium, such as theinteracion of HVC with galactic disks, the Parker instability, and the gas responseto the spiral density wave, alters considerably the \classic" results obtained in thethin disk picture of galactic disks which was popular in previous studies. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101027 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.10 |
| format | Artículo científico |
| id | redalyc_57101027 |
| institution | Redalyc |
| language | en |
| publishDate | 2001 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Some theoretical consequences of the thick, magnetized galactic disk Marco A. Martos Física, Astronomía y Matemáticas MHD GALAXY: HALO GALACTIC: STRUCTURE Some theoretical consequences of the thick, magnetized galactic disk Marco A. Martos Física, Astronomía y Matemáticas MHD GALAXY: HALO GALACTIC: STRUCTURE A number of recent observational studies reveal a new paradigm for diskgalaxies, one in which layers of warm ionized gas, dust structures and magneticelds commonly extend to considerable heights (of kpc) above their midplanes.This thick disk has an intricate and largely unknown structure. Its inclusion whilemodeling large scale dynamical processes in the interstellar medium, such as theinteracion of HVC with galactic disks, the Parker instability, and the gas responseto the spiral density wave, alters considerably the \classic" results obtained in thethin disk picture of galactic disks which was popular in previous studies. 2001 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101027 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.10 |
| title | Some theoretical consequences of the thick, magnetized galactic disk |
| topic | Física, Astronomía y Matemáticas MHD GALAXY: HALO GALACTIC: STRUCTURE |
| url | https://www.redalyc.org/articulo.oa?id=57101027 |