Spectroscopic study of galaxies in the Herschel Reference Sample
Contribuinte(s) |
Urrestilla Urizabal, Jon Gavazzi, Giuseppe Gorini, Giuseppe F. CIENCIA Y TECNOLOGIA ZIENTZIA ETA TEKNOLOGIA F. Grado en Física Fisikako Gradua |
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Data(s) |
28/04/2016
28/04/2016
28/04/2016
17/07/2015
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Resumo |
Galaxies are clusters of millions and billions of stars dynamically stable, with gas, dust and dark matter. They are the biggest isolated objects known in the Universe . Even though they are very complex systems, today we have a clear knowledge about their evolution and about their physical phenomena. Aside from the stellar component there is a gaseous component, principally neutral Hydrogen (HI), and dust that, although is not a significant component in terms of the mass, plays an important role on the absorption phenomena. Finally, cinematic and other kind of observations suggest the existence of a spheric dark matter halo, dominant in terms of mass and more extensive than the barionic component. |
Identificador |
http://hdl.handle.net/10810/18101 62905-656666-09 18231-656666 |
Idioma(s) |
eng es |
Direitos |
© 2015, el autor info:eu-repo/semantics/openAccess |
Palavras-Chave | #Herschel reference #galaxies #nuclear spectra |
Tipo |
info:eu-repo/semantics/bachelorThesis |