Tipo de publicación: Sin árbitro

  • Publicación
    The iron and oxygen abundances in the metal-poor star HD 140283 and in the Sun
    We present the results of a theoretical investigation of the impact of NLTE effects and of granulation inhomogeneities on the iron and oxygen abundances in the...
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    The irregular limb of Manoetius South Pole and Improved Orbital Solution (extended analysis)
    In 2033, after a 12-year trip across the Solar System, NASA's Lucy mission will arrive at the Patroclus─Menoetius binary system, in Jupiter's L5 cloud. On its...
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    The IRS Spitzer Spectra of the Magellanic Cloud Planetary Nebulae: Revealing the Dust and Gas Chemistry
    Planetary nebulae (PNe) in the Magellanic Clouds (LMC, SMC) offer a unique opportunity to study both the population and evolution of low- and intermediate-mass...
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    The ISO Survey of the Hubble Deep Field
    Not Available
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    The ISO Survey of the Hubble Deep Field
    Not Available
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    The Isolated Embedded Cluster GM 24
    GM 24 is a compact nebulous object immersed in the low-brightness HII region RCW 126. It is associated with a warm and dense CO cloud at whose centre a deeply...
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    The ISOPHOT Calibration Uplink System
    The planning of the ISOPHOT (Lemke et al. 1996) calibration during the Performance Verification (PV) phase, with its 4 day turn-around cycle, required mission...
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    The ISOPHOT Interactive Analysis (PIA)
    The ISOPHOT Interactive Analysis (PIA), originally conceived as a tool for ISOPHOT data processing to be used by calibration experts, rapidly became the...
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    The ISOPHOT Interactive Analysis PIA, a Calibration and Scientific Analysis Tool
    ISOPHOT is one of the instruments on board the Infrared Space Observatory (ISO), launched in November 1995 by the European Space Agency. ISOPHOT Interactive...