Mostrar el registro sencillo del ítem

dc.contributor.authorLisenfeld , Ute 
dc.contributor.authorEspada Fernández, Daniel 
dc.contributor.authorVerdes-Montenegro, L.
dc.contributor.authorKuno, N.
dc.contributor.authorAMIGA (team)
dc.date.accessioned2013-10-11T11:55:01Z
dc.date.available2013-10-11T11:55:01Z
dc.date.issued2009
dc.identifier.citationLisenfeld, U.; et al. Molecular gas properties of the most isolated galaxies [póster]. In: Conference "Galaxies in Isolation: exploring nature us nurture", Granada, may 12-15, 2009. [http://hdl.handle.net/10481/28422]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/28422
dc.description.abstractThe AMIGA project: The role of nature vs. nurture for the properties and evolution of galaxies is still an open question. In order to find answers, it is crucial to have a well-selected sample of isolated galaxies as a baseline and comparison. We built, refined and analised such a sample in the project AMIGA ("Analysis of the Interstellar Medium of Isolated GAlaxies”, http://www.iaa.es/AMIGA.html). The sample is based on the Catalogue of Isolated Galaxies (CIG) by Karanchenseva (1978) and the database (containing optical magnitude, Hα, far-infrared, radio continuum, HI and CO) enables us to characterize the properties of the star formation and interstellar medium.es_ES
dc.description.abstractThe CO data: We present CO data for 276 AMIGA galaxies, obtained to a large extent (189 galaxies) from own observations in addition to data from the literature. This sample enables us to characterize the molecular gas content of isolated galaxies.es_ES
dc.description.abstractComparison to other wavelengths: We show the comparison of the total molecular gas mass to the blue luminosity and the atomic gas mass. The molecular gas mass and the blue luminosity show a good correlation which can serve as a baseline to define the extected molecular gas content in a galaxy in the absence of interaction. The atomic gas mass is higher than the molecular gas mass for all Hubble types, and the ratio of the molecular-to-atomic mass ratio decreases towards late Hubble type.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.subjectMolecular gases_ES
dc.subjectGalaxies es_ES
dc.subjectIsolationes_ES
dc.titleMolecular gas properties of the most isolated galaxieses_ES
dc.typeinfo:eu-repo/semantics/otheres_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES


Ficheros en el ítem

[PDF]

Este ítem aparece en la(s) siguiente(s) colección(ones)

Mostrar el registro sencillo del ítem

Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License
Excepto si se señala otra cosa, la licencia del ítem se describe como Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License