activity
20072026
most citedOn the mass of ultra-light bosonic dark matter from galactic dynamics

90 citations · 355 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.GA2026

From blue to red spirals: Slow galaxy transformation via ram pressure stripping in TNG-50

V. Lora, J. I. Gonzalez-Carbajal, A. Pasquali +5

Late-type galaxies lose gas through ram-pressure stripping (RPS) after falling into a massive halo. Because this mechanism primarily removes the gaseous component while leaving the…

astro-ph.GA2024

Dark matter free dwarf galaxy formation at the the tips of the tentacles of jellyfish galaxies

V. Lora, R. Smith, J. Fritz +2

When falling into a galaxy cluster, galaxies experience a loss of gas due to ram pressure stripping. In particular, disk galaxies lose gas from their disks and very large tentacles…

astro-ph.SR2023

Shedding light on the ejection history of molecular outflows: Multiple velocity modes and precession

Veronica Lora, Thomas Nony, Alejandro Esquivel +1

Variable accretion has been well studied in evolved stages of low-mass stars formation. However, the accretion history in the initial phases of star formation is still a seldom stu…

astro-ph.SR2023★ 3 cited

Emerging planetary nebulae within 3D spiral patterns

V. Lora, J. A. Toalá, J. I. González-Carbajal +3

We present the first 3D radiation-hydrodynamic simulations of the formation of planetary nebulae (PNe) emerging from 3D spiral patterns. We use the GUACHO code to create 3D spiral…

astro-ph.SR2023★ 7 cited

XMM-Newton Detection of X-ray Emission from the Metal-Polluted White Dwarf G 29-38

S. Estrada-Dorado, M. A. Guerrero, J. A. Toalá +3

A recent analysis of Chandra X-ray data of the metal-polluted white dwarf (WD) G29-38 has revealed X-ray emission that can be attributed to the accretion of debris from a planetary…

astro-ph.GA2022★ 11 cited

The spatial distribution of globular clusters in dwarf spheroidal galaxies and the timing problem

F. J. Sanchez-Salcedo, V. Lora

The dynamical friction timescale of massive globular clusters (GCs) in the inner regions of cuspy dark haloes in dwarf spheroidal (dSph) galaxies can be much shorter than the Hubbl…