collaborators

5 papers

astro-ph.GA2026

Accurate inner stellar density slopes from projected surface densities in galaxies

Jorge Sanchez Almeida

The inner slope of the three-dimensional stellar density in dwarf galaxies (rho'[0]) is a sensitive probe of possible departures from the collisionless cold dark matter (CDM) parad…

astro-ph.GA2026

JWST spectra are consistent with the edge-on star-forming galaxy scenario for the "runaway supermassive black hole"

Jorge Sanchez Almeida, Ignacio Trujillo, Sebastian F. Sanchez +1

The linear structure reported by van Dokkum et al. (2023) has been proposed as either a massive stellar wake produced by a runaway supermassive black hole (SMBH) or a bulgeless edg…

astro-ph.GA2024

The stellar distribution in ultra-faint dwarf galaxies suggests deviations from the collision-less cold dark matter paradigm

Jorge Sanchez Almeida, Ignacio Trujillo, Angel R. Plastino

Unraveling the nature of dark matter (DM) stands as a primary objective in modern physics. Here we present evidence suggesting deviations from the collisionless Cold DM (CDM) parad…

astro-ph.GA2024

Einasto gravitational potentials have difficulty to hold spherically symmetric stellar systems with cores

Jorge Sanchez Almeida

It was known that an ideal spherically symmetric stellar system with isotropic velocities and an inner core cannot reside in a Navarro, Frenk, and White (NFW) gravitational potenti…

astro-ph.GA2024

Deep HST imaging favors the bulgeless edge-on galaxy explanation for the hypothetical stellar wake created by a runaway supermassive black hole

Mireia Montes, Jorge Sánchez Almeida, Ignacio Trujillo

A long linear structure recently discovered could be the stellar wake produced by the passage of a runaway supermassive black hole (SMBH) or, alternatively, a bulgeless edge-on gal…