New observations reveal that the highly variable winds arising from the accretion disk at the center of the active galaxy NGC 5548 are linked to the large changes in the galaxy’s X-ray flux.
Accretion disks around rogue intermediate-mass black holes are a potential explanation for the double-peaked hydrogen emission lines observed in gas clouds in galaxies in the local universe.
Transit observations can’t say which star in a binary system hosts a transiting exoplanet, but models can help; in one study, 70% of sampled transiting planets orbited the primary star in the system.
Pitted impact deposits within craters are spectrally distinct from those in crater ejecta, potentially due to oxidation processes, meaning that these regions are different in ways apart from space weathering.
Simulations suggest that the inner solar system planets would not be directly exposed to the blast wave of a nearby supernova, suggesting that supernova material on Earth came in the form of dust, not plasma.
Researchers attempt to discern why the plasma of solar active regions has a different composition than the surrounding solar surface, finding that the reasons are complex and likely evolve as the active region evolves.