Photoionization and electron–ion recombination in astrophysical plasmas
DJ Hillier - Atoms, 2023 - mdpi.com
Photoionization and its inverse, electron–ion recombination, are key processes that
influence many astrophysical plasmas (and gasses), and the diagnostics that we use to …
influence many astrophysical plasmas (and gasses), and the diagnostics that we use to …
Magnetic imprisonment of dusty pinballs by a supernova remnant
BJ Fry, BD Fields, JR Ellis - The Astrophysical Journal, 2020 - iopscience.iop.org
Motivated by recent measurements of deposits of 60 Fe on the ocean floor and the lunar
surface, we model the transport of dust grains containing 60 Fe from a near-Earth (ie, within …
surface, we model the transport of dust grains containing 60 Fe from a near-Earth (ie, within …
Dust and gas in the central region of NGC 1316 (Fornax A)-Its origin and nature
T Richtler, M Hilker, E Iodice - Astronomy & Astrophysics, 2020 - aanda.org
Context. The early-type galaxy NGC 1316, associated with the radio source Fornax A, hosts
about 10 7 M⊙ of dust within a central radius of 5 kpc. These prominent dust structures are …
about 10 7 M⊙ of dust within a central radius of 5 kpc. These prominent dust structures are …