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Supernovae: Where and why do they break off?
(SABER ULA, 2005)
Supernovae: Where and why do they break off?
(SABER ULA, 2005)
The x-ray luminosity functions of field low-mass x-ray binaries in early-type galaxies: evidence for a stellar age dependence
(UNIVERSITY OF CHICAGO PRESS, 2014)
Luminosity functions of LMXBs in different stellar environments
(2011)
Aims. Based on the archival data from the Chandra observations of nearby galaxies, we study different sub populations of low-mass X-ray binaries (LMXBs) – dynamically formed systems in globular clusters (GCs) and in the ...
Análise de populações estelares e subestruturas em aglomerados de galáxias
(Universidade Federal de Santa MariaBRFísicaUFSMPrograma de Pós-Graduação em Física, 2015-08-25)
In this work, we investigated differences between stellar populations of galaxies that are part
of a cluster with and without substructures. We used optical spectra obtained from Sloan Digital
Sky Servey III DR10 for the ...
The rest-frame optical (900nm) galaxy luminosity function at z∼4–7: abundance matching points to limited evolution in the MSTAR/MHALO ratio at z ≥ 4
(IOP Publishing Ltd., 2017)
We present the first determination of the galaxy luminosity function (LF) at z ∼4, 5, 6, and 7, in the rest-frame
optical at l ~ rest 900 nm (z′ band). The rest-frame optical light traces the content in low-mass evolved ...