We present a kpc-scale analysis of the relationship between the molecular depletion time (τ^mol_dep) and the orbital time (τorb) across the field of 39 face-on...
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PublicaciónThe EDGE-CALIFA survey: the influence of galactic rotation on the molecular depletion time across the Hubble sequence
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PublicaciónThe EDGE–CALIFA Survey: Variations in the Molecular Gas Depletion Time in Local Galaxies
We present results from the EDGE survey, a spatially resolved CO(1‑0) follow-up to CALIFA, an optical Integral Field Unit survey of local galaxies. By combining...
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PublicaciónThe effect of environment on star forming galaxies at redshift 1 First insight from PACS (Corrigendum)
Not Available
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PublicaciónThe effect of environment on star forming galaxies at redshift. I. First insight from PACS
We use deep 70, 100 and 160 μm observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS...
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PublicaciónThe effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
Recent observational and theoretical studies indicate that the stellar initial mass function (IMF) varies systematically with the environment (star formation...
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PublicaciónThe ELMER Detection Subsystem
ELMER is a multi-purpose instrument for the GTC designed for both, imaging and spectroscopy in the visible range. The detection subsystem consists of a single...
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PublicaciónThe embedded cluster IRAS17136 - 3617 associated with the nebulosity GM24
Radio, infrared, and optical observations of the embedded infrared cluster IRAS17136 - 3617 are reviewed. The cluster consists of more than 25 stars with a...
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PublicaciónThe EROs at z < 1.5 in the Groth-Westphal field of the GOYA survey
The study of the Extremly Red Objects (EROs), is the importance for setting constraints on the first epoch of massive galaxy formation, for exploring the...
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PublicaciónThe evolution of compact massive quiescent and star-forming galaxies derived from the R<SUB>e</SUB>-R<SUB>h</SUB> and M<SUB>star</SUB>-M<SUB>h</SUB> relations
The mean size (effective radius R e) of massive galaxies (MGs; M star > 10 11.2M ⊙) is observed to increase steadily with cosmic time. It is still unclear...