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dc.contributor.authorGALEX Team
dc.contributor.editorKurtz, S.
dc.contributor.editorFranco, J.
dc.contributor.editorHong, S.
dc.contributor.editorGarcia-Segura, G.
dc.contributor.editorSantillan, A.
dc.contributor.editorKim, J.
dc.contributor.editorHan, I.
dc.date.accessioned2014-05-28T09:00:27Z
dc.date.available2014-05-28T09:00:27Z
dc.date.issued2007
dc.identifier.citationGALEX Team 2007 , The star formation history of early-type galaxies . in S Kurtz , J Franco , S Hong , G Garcia-Segura , A Santillan , J Kim & I Han (eds) , The 3rd Mexico-Korea Conference on Astrophysics : Telescopes of the Future and San Pedro Martir . vol. 28 , Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias , vol. 28 , Instituto de Astronomía, UNAM , pp. 109-112 , The third Mexico-Korea conference on astrophysics: telescopes of the future and San Pedro Martir , Mexico City , Mexico , 8/11/05 .
dc.identifier.citationconference
dc.identifier.isbn9789703232734
dc.identifier.otherORCID: /0000-0002-5601-575X/work/77850220
dc.identifier.urihttp://hdl.handle.net/2299/13553
dc.description.abstractThe UV light is an effective tracer for young stars. Base on the recent GALEX UV data of nearby, bright early-type galaxies, we find that 30% of them show a UV flux that is too strong to explain without invoking a 1-3% (in total stellar mass) star formation rate in the last billion years. This implies that low-level residual star formation was common during the last few billion years even in bright, early-type galaxies. We discuss the implications for the formation and evolution of early-type galaxies. This article is a summary of our recent work (Yi et al. 2005; Schawinski et al. 2006; Kaviraj et al. 2006).en
dc.language.isoeng
dc.publisherInstituto de Astronomía, UNAM
dc.relation.ispartofThe 3rd Mexico-Korea Conference on Astrophysics
dc.relation.ispartofseriesRevista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
dc.titleThe star formation history of early-type galaxiesen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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