Tipo de publicación: Sin árbitro

  • Publicación
    Precise abundances of Mg and neutron-capture elements in the Milky Way: chemodynamical relations using Gaia data and chemical evolution models
    The abundance of alpha and neutron-capture elements provide an important fossil signature in Galactic archaeology for tracing the chemical evolution of the...
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    Precise seismology with TESS CVZ data
    The release of TESS light-curves gives us the opportunity to perform all-sky seismology for a lot of stars. Among them, the higher quality data that was...
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    Precise surface gravitites of A-type stars from Asteroseismology
    δ Sct are one of the most abundant pulsating stars in our Galaxy. In addition, they have moderate to fast rotations and periods of several hours. That makes...
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    Precise X-ray position of A1744-36 (=XTE J1748-361?)
    The Ariel-5 X-ray transient A1744-36 and the newly-discovered transient XTE J1748-361 may be identical (ATEL #204). Based on a 16 ks Chandra ACIS-S observation...
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    Precision Limitations of Radial Velocity Measurements of the Active Red Giants in the Penn State-Torun Planet Search
    Not Available
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    Predicted x-ray backgrounds for the International X-ray Observatory
    The background that will be observed by IXO's X-ray detectors naturally separates into two components: (1) a Cosmic X-ray Background (CXB), primarily due to...
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    Predicting Radio Activity in X-ray Binaries with Optical/Infrared Monitoring
    X-ray binaries undergo outbursts due to increased mass accretion rate in the disc towards the compact object, a black hole or neutron star. Recently, a picture...
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    Predicting Space Weathering Effects on Primitive Asteroids (101955) Bennu and (162173) Ryugu
    Two sample-return missions, OSIRIS-REx and Hayabusa 2, have just arrived at primitive near-Earth asteroids (NEAs) (101955) Bennu and (162173) Ryugu, and it is...
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    Prediction of close binarity based on nebula morphology
    A thorough search of the OGLE-III microlensing project has more than doubled the total sample of PNe known to have close binary central stars. These discoveries...