Publicación
Starbursts and Galaxy Evolution: results from COSMOS survey.
The search for starbursts galaxies in COSMOS database by a tailored procedure that uses the photometry from SUBARU, results in 220 targets at z
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PublicaciónStarbursts Are Preferentially Interacting: Confirmation from the Nearest GalaxiesWe complement a recent Letter by Luo et al. by comparing the fraction of starburst galaxies that are interacting with the overall fraction of interacting...
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PublicaciónStars at Low Metallicity in Dwarf GalaxiesDwarf galaxies offer an opportunity to understand the properties of low metallicity star formation both today and at the earliest times at the epoch of the...
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PublicaciónStatistical Properties of Circumnuclear H II Regions in Nearby GalaxiesWe analyze the statistical properties of the circumnuclear H II regions of a sample of 52 nearby galaxies (v
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PublicaciónStatistical properties of H II regions in the disc of M100From a new mosaic image in the Hα line of the complete disc of the spiral galaxy M100, a catalogue is composed listing 1948 individual H II regions. I give...
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PublicaciónStatistical Properties of Highly Luminous HII Regions in the Interacting Zone of the Antennae Galaxies, and Comparison with the Molecular Cloud ComponentWe have used the package CLOUDPROPS (Rosolowsky & Leroy 2008) in order to identify clouds, which are contained in data cubes of molecular/Hα line emission, and...
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PublicaciónStatistical redshift of the very-high-energy blazar S5 0716+714Context. Blazars are the most numerous class of very-high-energy (VHE; E > 100 GeV) gamma-ray emitters. At present, measured redshifts are available only for...
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PublicaciónStatistical studies of HII regions in nearby galaxies. I. Spitzer near-IR luminosities and temperatures, compared with Hα luminosities, from selected HII regions in M100Aims: We systematically study the relations between the Hα luminosity and the near-IR luminosity and temperature of a set of selected HII regions in the disc of...
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PublicaciónStatistical Synthesis ModelsIn this contribution we evaluate the minimal cluster mass for which the effects of an incomplete sampling of the Initial Mass Function (IMF) cannot be neglected...