113 citations · 311 across the 14 of their papers we have counts for
14 papers
Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension
Prachi Prajapati, Axel Weiss, Dominik Riechers +17
The CO luminosity-to-H mass conversion factor () remains a debated uncertainty in determining molecular gas masses of high-redshift dusty star-forming galaxies (DSFGs).…
The Impact of Seyfert Jets on Galaxy Evolution Across Major Scaling Relations
Julianne Goddard, Isaac Shlosman, Emilio Romano-Diaz
We analyze a suite of high-resolution cosmological zoom-in simulations of jetted Seyfert galaxies over projected on the major scaling relations, comparing trajectories of…
Modeling Cosmological Evolution of Jetted Seyfert Galaxies for z<10
Julianne Goddard, Isaac Shlosman, Emilio Romano-Diaz
We use high-resolution cosmological zoom-in simulations to model mechanical and thermal feedback from AGN onto the evolution of Seyfert-type galaxies, studying the morphology of ce…
The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
Prachi Khatri, Emilio Romano-Díaz, Cristiano Porciani
The [C II] fine-structure line at 157.74 m is one of the brightest far-infrared emission lines and an important probe of galaxy properties like the star formation rate (SFR) and…
Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
Da Bi, Isaac Shlosman, Emilio Romano-Diaz
We use high-resolution zoom-in simulations to study the fueling of the central galaxies by gas accretion from cosmological filaments at high redshifts, z>=2. Their parent haloes wi…
Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
Yvonne A. Fichtner, Luca Grassitelli, Emilio Romano-Díaz +1
We compute different sets of stellar evolutionary tracks in order to quantify the energy, mass, and metals yielded by massive main-sequence and post-main-sequence winds. Our aim is…