Dust grain size distributions evolve from large-grain dominated at high redshift to MRN-like at low redshift, driven primarily by shattering and ISM accretion after stars supply initial large grains, reproducing z=0 dust masses and Milky Way extinction properties.
M., Hendriks, D., Vijayan, A
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.GA 3roles
background 1polarities
background 1representative citing papers
A unified JSONL/CSV corpus merges photometric, kinematic, dynamical, and chemical parameters for all 174 Milky Way globular clusters from Harris, Gaia EDR3, Baumgardt N-body, and APOGEE DR17 surveys.
The paper reviews dust production, destruction and growth processes in galaxies, compiles literature data on comoving dust mass density, presents evidence for and against interstellar dust growth, and identifies the high-redshift dust budget as needing further study.
citing papers explorer
-
Dust and Grain Size Evolution in Galaxy Simulations: What Matters and What Does Not
Dust grain size distributions evolve from large-grain dominated at high redshift to MRN-like at low redshift, driven primarily by shattering and ISM accretion after stars supply initial large grains, reproducing z=0 dust masses and Milky Way extinction properties.
-
A Multi-Survey Machine-Readable Corpus of Milky Way Globular Cluster Parameters for Retrieval-Augmented Generation Applications
A unified JSONL/CSV corpus merges photometric, kinematic, dynamical, and chemical parameters for all 174 Milky Way globular clusters from Harris, Gaia EDR3, Baumgardt N-body, and APOGEE DR17 surveys.
-
Interstellar dust production, destruction and effects of dust depletion in galaxies
The paper reviews dust production, destruction and growth processes in galaxies, compiles literature data on comoving dust mass density, presents evidence for and against interstellar dust growth, and identifies the high-redshift dust budget as needing further study.