Spectroscopic study of galaxies in the Herschel Reference Sample


Autoria(s): Fernández Otegui, Jon
Contribuinte(s)

Urrestilla Urizabal, Jon

Gavazzi, Giuseppe

Gorini, Giuseppe

F. CIENCIA Y TECNOLOGIA

ZIENTZIA ETA TEKNOLOGIA F.

Grado en Física

Fisikako Gradua

Data(s)

28/04/2016

28/04/2016

28/04/2016

17/07/2015

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