Publication type: Non-refereed

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    Theoretical models in the Virtual Observatory
    Although full interoperability between theoretical and observational data in the framework of the Virtual Observatory would be a very desirable achievement, the...
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    Theory and observations of a jet in the σ Orionis region: HH 444
    The discovery of a system of Herbig-Haro objects ejected by young, low mass stars in the &sigma Orionis region (Reipurth et al. 1998) has given rise to models...
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    Theory for the Nonlinear Ultrafast Dynamics of Small Clusters after Ionization
    The ultrafast relaxation of small clusters immediately after ionization is studied. For small Hg$_n$ clusters we determine the fragmentation-time distributions...
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    Theory for the Ultrafast Structural Response of optically excited small clusters: Time-dependence of the Ionization Potential
    Combining an electronic theory with molecular dynamics simulations we present results for the ultrafast structural changes in small clusters. We determine the...
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    Theory, Observation, and Modeling of the Zeeman and Paschen-Back Effects in Molecular Lines
    We present a historical review of the theory of the Zeeman effect in molecular lines, from its discovery at the end of the 19th century till today. The fast...
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    Thermal and mechanical design and test of the CCD mount for the WEAVE spectrograph cryostats
    WEAVE is the new multi-object spectrograph for the William Herschel Telescope on La Palma. The culmination of prime focus, the large number of fibers and the...
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    Thermal and Non-Thermal Components of the X-Ray Emission from Jupiter
    Recent XMM-Newton and Chandra observations have revealed that Jupiter's X-ray emission comprises both, thermal and non-thermal spectral components. While the...
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    Thermal design and performance of the balloon-borne large aperture submillimeter telescope for polarimetry BLASTPol
    We present the thermal model of the Balloon-borne Large-Aperture Submillimeter Telescope for Polarimetry (BLASTPol). This instrument was successfully own in two...
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    Thermal Dust Imaging of Massive Star-Forming Regions: W3 Main and W3 (OH)
    We present the preliminary results of mid-infrared images at 8.7, 9.7 and 12.5 micron of the complex massive star formation regions W3 Main and W 3(OH).