Publication type: Non-refereed

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    Planet candidates orbiting the Barnard's star seen with ESPRESSO
    ESPRESSO is the VLT ultra-stable high-resolution spectrograph, developed by institutions from Switzerland, Italy, Portugal, Spain, and ESO, located in the...
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    Planet Detection Capabilities of the Eddington Mission
    Not Available
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    Planet erosion by coronal radiation
    According to theory, high energy emission from the coronae of cool stars can severely erode the atmosphere of orbiting planets. To test the long term effects of...
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    Planet Formation Imager (PFI): science vision and key requirements
    The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of...
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    Planet formation imager: project update
    The Planet Formation Imager (PFI) is a near- and mid-infrared interferometer project with the driving science goal of imaging directly the key stages of planet...
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    Planetary and Proto-Planetary Nebulae in the IRAS Two-Colour Diagram
    Not Available
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    Planetary Nebula candidates in a region of M 33
    We detect some objects that can be classified as planetary nebulae candidate s (PNc), using images of a southern region of M 33. This search is the deepest one...
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    Planetary Nebula Candidates in a Region of M33
    Planetary nebulae (PNe) have been used to trace the chemical evolution of galaxies, not only in the Milky Way (Esteban & Peimbert 1995 and references therein)...
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    Planetary nebula LoTr5: hints of a possible third companion in a long-period binary central star
    LoTr 5 is a planetary nebula with an unusual long-period binary central star. The pair consists of a rapidly rotating G-type star and a hot star, which is...