16 citations · 21 across the 5 of their papers we have counts for
7 papers
Dust at cosmic dawn: unveiling the onset of dust and obscured star formation at
Hiddo Algera, Tom Bakx, Manuel Aravena +31
Although less than 1 percent of the baryonic mass budget of a galaxy, cosmic dust profoundly alters the multi-wavelength appearance of galaxies across cosmic time. The (sub)millime…
When dust growth takes over: the origin of dust in post-reionization galaxies
Omima Osman, Gabriella De Lucia, Andreas. L. Faisst +3
The post-reionization epoch (-6) marks a critical phase in galaxy evolution, during which galaxies rapidly assemble their stellar mass, enrich their interstellar medium, an…
Dust evolution across cosmic times as seen through DUSTY-GAEA
Omima Osman, Gabriella De Lucia, Fabio Fontanot +2
For many decades, dust has been recognised as an important ingredient in galaxy formation and evolution. This paper presents a novel self-consistent implementation of dust formatio…
The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~5
Andreas L. Faisst, Lun-Jun Liu, Yohan Dubois +54
We present the stellar mass-metallicity relation (MZR) and mass-metallicity-star formation relation ("fundamental metallicity relation"; FMR) of 18 massive (log(M/Msun) = 9.5 - 11)…
Photoelectric heating effects on the evolution of luminous disk galaxies
Omima Osman, Kenji Bekki, Luca Cortese
Photoelectric heating (PEH) influences the temperature and density of the interstellar medium (ISM), and potentially also affecting star formation. PEH is expected to have a strong…
The role of dust destruction and dust growth in the evolution of the interstellar medium
Omima Osman, Kenji Bekki, Luca Cortese
We use Milky Way-like chemodynamical simulations with a new treatment for dust destruction and growth to investigate how these two processes affect the properties of the interstell…
Strong suppression of star formation and spiral arm formation in disk galaxies with counter-rotating gas disks
Omima Osman, Kenji Bekki
Galaxy-wide star formation can be quenched by a number of physical processes such as environmental effects (e.g., ram pressure stripping) and supernova feedback. Using numerical si…