Afficher la notice abrégée

dc.contributor.authorOcaña Flaquer, Breezy
dc.contributor.authorLeon, S.
dc.contributor.authorEspada Fernández, Daniel 
dc.contributor.authorMartín Ruiz, Sergio
dc.contributor.authorLisenfeld , Ute 
dc.contributor.authorVerley, Simon 
dc.contributor.authorSabater, J.
dc.contributor.authorVerdes-Montenegro, L.
dc.date.accessioned2013-10-09T10:20:04Z
dc.date.available2013-10-09T10:20:04Z
dc.date.issued2009
dc.identifier.citationOcaña Flaquer, B.; et al. Does the LFIR-LHCN correlation hold for low LFIR isolated galaxies?. In: Verdes-Montenegro, L; Olmo, A. y Sulentic, J. (eds.) Galaxies in Isolation: exploring nature versus nature. San Francisco (USA): Astronomical Society of the Pacific, 2010. p. 274. (Conference Series, 421). [http://hdl.handle.net/10481/28387]es_ES
dc.identifier.isbn978-1-58381-722-3
dc.identifier.isbn978-1-58381-723-0
dc.identifier.issn1050-3390
dc.identifier.otherarXiv:0909.4192v1
dc.identifier.urihttp://hdl.handle.net/10481/28387
dc.descriptionInternational conference “Galaxies in Isolation: Exploring Nature vs. Nurture” held in Granada (Spain), May 12–15, 2009.es_ES
dc.description.abstractLow LFIR Isolated Galaxies (IGs) from the AMIGA sample have low level of Star Formation (SF) activity. We observed the HCN(1-0) emission in a sample of IGs in order to test whether they follow the tight relation between LHCN and LFIR found for galaxies with more active SF.es_ES
dc.language.isoenges_ES
dc.publisherAstronomical Society of the Pacifices_ES
dc.relation.ispartofseriesConference Series;421
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs 3.0 Licensees_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es_ES
dc.subjectIsolatedes_ES
dc.subjectGalaxies es_ES
dc.titleDoes the LFIR-LHCN correlation hold for low LFIR isolated galaxies?es_ES
dc.typeconference outputes_ES
dc.rights.accessRightsopen accesses_ES


Fichier(s) constituant ce document

[PDF]

Ce document figure dans la(les) collection(s) suivante(s)

Afficher la notice abrégée

Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License
Excepté là où spécifié autrement, la license de ce document est décrite en tant que Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License