Publication type: Non-refereed

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    How do massive stars form? Finding targets for MIRADAS
    Observations from massive stars in H II regions can help to clarify theories of massive star formation because they show the degree of isolation under which...
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    How does breakup influence near-barrier fusion of weakly bound light nuclei ?
    The influence on the fusion process of coupling to collective degrees of freedom has been explored. The significant enhancement of he fusion cross setion at sub...
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    How Fast the Nucleus of Comet Hale-Bopp was Rotating?
    At the First International Conference on Comet Hale-Bopp (Canaries, 1998) many astronomers agreed with the value of the period of axial rotation of its nucleus...
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    How have the massive galaxies evolved over cosmic time
    Not Available
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    How Hot are Hot Stars?: New Temperatures for mid-O types from FUSE data
    We 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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    How 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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    How massive galaxies have evolved over cosmic time?
    Not Available
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    How Normal Disk Galaxies Ionize their Surroundings
    We 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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    How Planetary Nebulae Shells Interact with their Local Environement
    Planetary Nebula (PN) shells and AGB circumstellar envelopes evolve under a wide range of external conditions, from the high ISM densities found in the Galactic...