Publicación
How have the massive galaxies evolved over cosmic time
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PublicaciónHow Hot are Hot Stars?: New Temperatures for mid-O types from FUSE dataWe analysed high resolution spectra of Galactic O-type stars from the far-UV to the optical. We combined spectra from the Far Ultraviolet Spectroscopic Explorer...
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PublicaciónHow Important is Rotational Fission in the Trans-Neptunian Region?We introduce the idea that rotational fission is a possible mechanism in the formation of systems of large TNOs: binary systems, complex systems (Haumea), and...
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PublicaciónHow massive galaxies have evolved over cosmic time?Not Available
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PublicaciónHow Normal Disk Galaxies Ionize their SurroundingsWe examine using numerical examples and conservative assumptions, the consequences of the fractal structure of the interstellar medium in a disk galaxy in...
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PublicaciónHow Planetary Nebulae Shells Interact with their Local EnvironementPlanetary Nebula (PN) shells and AGB circumstellar envelopes evolve under a wide range of external conditions, from the high ISM densities found in the Galactic...
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PublicaciónHow simple are galaxies?Not Available
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PublicaciónHow the most highly luminous H II regions in galaxies ionize the interstellar and intergalactic media.Not Available
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PublicaciónHow to observe with GTCWe present here the outline of the process that any potential GTC observer will need to follow in order to perform their observations. Depending on which of the...