dc.contributor.advisor | Urrestilla Urizabal, Jon | es |
dc.contributor.advisor | Gavazzi, Giuseppe | es |
dc.contributor.advisor | Gorini, Giuseppe | es |
dc.contributor.author | Fernández Otegui, Jon | es |
dc.contributor.other | F. CIENCIA Y TECNOLOGIA | es |
dc.contributor.other | ZIENTZIA ETA TEKNOLOGIA F. | eu |
dc.date.accessioned | 2016-04-28T18:52:09Z | |
dc.date.available | 2016-04-28T18:52:09Z | |
dc.date.issued | 2016-04-28 | |
dc.identifier.uri | http://hdl.handle.net/10810/18101 | |
dc.description.abstract | 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. | es |
dc.language.iso | eng | es |
dc.rights | info:eu-repo/semantics/openAccess | es |
dc.subject | Herschel reference | es |
dc.subject | galaxies | es |
dc.subject | nuclear spectra | es |
dc.title | Spectroscopic study of galaxies in the Herschel Reference Sample | es |
dc.type | info:eu-repo/semantics/bachelorThesis | es |
dc.date.updated | 2015-07-17T12:16:24Z | es |
dc.language.rfc3066 | es | es |
dc.rights.holder | © 2015, el autor | es |
dc.contributor.degree | Grado en Física | es |
dc.contributor.degree | Fisikako Gradua | es |
dc.identifier.gaurregister | 62905-656666-09 | es |
dc.identifier.gaurassign | 18231-656666 | es |