The authors produce a 3D tomographic reconstruction of Galactic cosmic-ray proton density from Fermi-LAT gamma-ray data and a gas model, finding a smooth distribution with moderate inner-Galaxy enhancement consistent with AMS-02 local measurements.
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6 Pith papers cite this work. Polarity classification is still indexing.
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MWC 656 hosts a hot stripped star companion of 1.48 solar masses instead of a black hole.
Identifies 596 WD-MS binary candidates within 100 pc (497 new) by detecting NUV excess in Gaia sources and fitting SEDs to estimate WD temperatures and masses.
Long-term polarimetric monitoring shows circumstellar disks in Be/X-ray binaries are smaller and denser than in isolated Be stars, with distortions often preceding giant X-ray outbursts.
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.
Planet-hosting wide binaries display diverse differential abundance trends with condensation temperature that are not universal across systems.
citing papers explorer
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A Three-Dimensional Tomographic Reconstruction of the Galactic Cosmic-Ray Proton Density
The authors produce a 3D tomographic reconstruction of Galactic cosmic-ray proton density from Fermi-LAT gamma-ray data and a gas model, finding a smooth distribution with moderate inner-Galaxy enhancement consistent with AMS-02 local measurements.
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Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
MWC 656 hosts a hot stripped star companion of 1.48 solar masses instead of a black hole.
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Revealing Unresolved White Dwarf-Main Sequence Binaries using Gaia DR3 and GALEX I. A Volume limited study of 100 pc
Identifies 596 WD-MS binary candidates within 100 pc (497 new) by detecting NUV excess in Gaia sources and fitting SEDs to estimate WD temperatures and masses.
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Long-term optical variability of high-mass X-ray binaries. III. Polarimetry
Long-term polarimetric monitoring shows circumstellar disks in Be/X-ray binaries are smaller and denser than in isolated Be stars, with distortions often preceding giant X-ray outbursts.
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Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.
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Chemical signatures of planetary systems in their host stars. Near-infrared spectroscopy of four planet-hosting wide binaries
Planet-hosting wide binaries display diverse differential abundance trends with condensation temperature that are not universal across systems.