Tipo de publicación: Sin árbitro

  • Publicación
    The Photometric Light Curves Of Earth As A Planet Along Its History
    By making use of real information about the continental and oceanic surface distribution of the Earth, and cloudiness data from the International Satellite...
  • Publicación
    The photometric properties and stellar populations in extremely red galaxies
    We study the morphology and masses of extremely red galaxies (EROs) within the GOYA survey (Galaxy Origins and Young Assembly), by combining optical data (UBVI)...
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    The physical nature of asteroids in cometary orbit
    Asteroids in cometary orbits can be defined as minor planets that do not present cometary activity and has orbits with Tisserand parameter T 3 (typical of...
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    The Physical Parameters and Excitation of Jets and Knots in PNe
    We are carrying out a study of the physical parameters and excitation of low-ionization structures (LIS) in planetary nebulae (PNe). Since the optical...
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    The Physical Properties of the Near Earth Asteroids 2005 UD and 2001 SG286
    Research into the orbital and physical properties near-Earth asteroids (NEAs) is important as these objects can reveal information about the origin and history...
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    The physics of the HII regions: the photoionization equilibrium in the HII regions of M51
    A general overview of the physical properties of the HII regions is presented here, emphasizing the various general models made to explain their structure and...
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    The physics of the solar core deduced from GOLF and MDI acoustic modes
    We use the recent results on solar acoustic modes coming from GOLF and MDI, to demonstrate that we improve the quality of the inversion of the sound speed and...
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    The pier and building of the European Solar Telescope (EST)
    EST (European Solar Telescope) is a 4-m class solar telescope, which is currently in the conceptual design phase. EST will be located in the Canary Islands and...
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    The plague of magnetic spots among the hot stars of globular clusters: a bridge between MS and WD stars
    I will report on our recent discovery of a wide-spread photometric variability among hot (~20,000 – 30,000 K) extreme horizontal branch (EHB) stars in Galactic...