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AMIGA: HI content of the mos isolated galaxies

dc.contributor.authorEspada Fernández, Daniel 
dc.contributor.authorVerdes-Montenegro, L.
dc.contributor.authorLeon, S.
dc.contributor.authorLisenfeld , Ute 
dc.contributor.authorHuchtmeier, W.
dc.contributor.authorVerley, Simon 
dc.contributor.authorSabater, J.
dc.contributor.authorGarcía, E.
dc.date.accessioned2013-10-15T08:12:44Z
dc.date.available2013-10-15T08:12:44Z
dc.date.issued2004
dc.identifier.citationEspada, D.; et al. AMIGA: HI content of the mos isolated galaxies. In: Meeting "The many scales of the Universe JENAM", Granada (Spain) september 2004. [http://hdl.handle.net/10481/28430]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/28430
dc.description.abstractWe present an analysis of the atomic gas (HI) properties for a large sample of isolated galaxies. It includes nearly 800 isolated galaxies, members of the Catalogue of Isolated Galaxies (CIG, Karachentseva 1973). Since the number of objects in our sample is much larger than any HI data compilation of really isolated galaxies presented before, we will be able to improve substantially the statistical studies done up to now. The data have been obtained both from the bibliography and by our own observations, done by means of the Nançay, Effelsberg, Arecibo and GBT radio-telescopes.es_ES
dc.language.isoenges_ES
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs 3.0 Licensees_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es_ES
dc.subjectAMIGA (Analysis of the interstellar Medium of Isolated Galaxies)es_ES
dc.subjectGalaxies es_ES
dc.subjectIsolatedes_ES
dc.subjectPósteres_ES
dc.subjectAtomic gas (HI)es_ES
dc.subjectCatalogue of Isolated Galaxies (CIG)es_ES
dc.titleAMIGA: HI content of the mos isolated galaxieses_ES
dc.typeotheres_ES
dc.rights.accessRightsopen accesses_ES


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