activity
20232026
most citedSimulated observations of star formation regions: infrared evolution of globally collapsing clouds

10 citations · 12 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2026

Modeling (Sub-)millimeter Scattering Properties of Fractal and Consolidated Porous Particles: Applications to Protoplanetary Disks

Gonzalo Vargas, Daniel Guirado, Carlos Carrasco-Gonzalez +5

We perform light-scattering numerical simulations for two dust populations: (i) consolidated porous particles computed with the discrete dipole approximation (ADDA) and (ii) highly…

astro-ph.SR2026★ 1 cited

Exploring Polarized Millimeter Emission from Protoplanetary Disks with Irregular Dust Grains

Jesús Miguel Jáquez-Domínguez, Carlos Carrasco-González, Daniel Guirado +4

Polarization at millimeter wavelengths provides a powerful diagnostic of dust grain properties in protoplanetary disks. Standard models based on solid spherical grains often strugg…

astro-ph.GA2025★ 1 cited

ngVLA Synthetic Observations of Ionized Gas in Massive Protostars

Jesús M. Jáquez-Domínguez, Roberto Galván-Madrid, Alfonso Trejo-Cruz +11

Massive star formation involves significant ionization in the innermost regions near the central object, such as gravitationally trapped H II regions, jets, ionized disks, or winds…

astro-ph.IM2024

Next Generation Very Large Array Memo #122: Characterization of the synthesized beam with and without MID antennas in Mexico

Alfonso Trejo-Cruz, Roberto Galván-Madrid, Carlos Carrasco-González +5

Synthesized beam (PSF) synthetic observations with and without the antennas in Mexico are analyzed. For a simple continuum observing setup, we generated visibility files and their…

astro-ph.GA2023★ 10 cited

Simulated observations of star formation regions: infrared evolution of globally collapsing clouds

Jesús M. Jáquez-Domínguez, Roberto Galván-Madrid, Jacopo Fritz +6

The direct comparison between hydrodynamical simulations and observations is needed to improve the physics included in the former and test biases in the latter. Post-processing rad…