activity
19982022
most citedOptical and Infrared photometry of the type IIn SN 1998S:Days 11-146

168 citations · 359 across the 14 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2022★ 2 cited

Virial masses of late type galaxies from the SDSS DR16

A. Nigoche-Netro, E. de la Fuente, R. J. Diaz +6

Motivated by the challenges of calculating the dynamical masses of late-type galaxies (LTGs) and the enormous amount of data from the Sloan Digital Sky Survey (SDSS), we calculate…

astro-ph.GA2020★ 7 cited

Ultracompact HII regions with extended emission: The case of G43.89-0.78 and its molecular environment

Eduardo de la Fuente, Daniel Tafoya, Miguel A. Trinidad +6

The Karl Jansky Very Large Array (VLA), Owens Valley Radio Observatory (OVRO), Atacama Large Millimetric Array (ALMA), and the infrared \textit{Spitzer} observatories, are powerful…

astro-ph.GA2020

Study of galaxy morphology and merging time of two interacting galaxies under different initial rotation and orientation configurations

Elkin L. Lopez, Gustavo V. Lopez, Simon N. Kemp

Using the GADGET-2 N-body code, we make a study of the galaxy morphology and merging time due to two interacting galaxies (for the same types and different sizes and masses, …

astro-ph.GA2019★ 15 cited

Ultracompact H II Regions with Extended Emission: The Complete View

Eduardo de la Fuente, Alicia Porras, Miguel A. Trinidad +5

In this paper we present the results of a morphological study performed on a sample of 28 ultracompact \hiirs~located near extended free-free emission, using radio continuum observ…

astro-ph.GA2019★ 6 cited

The quantity of dark matter in early-type galaxies and its relation to the environment

A. Nigoche-Netro, G. Ramos-Larios, P. Lagos +5

We study the behavior of the dynamical and stellar mass inside the effective radius of early-type galaxies (ETGs) as a function of environment considering Newtonian dynamics, diffe…

astro-ph.GA2019

Analytical model for the dynamical motion of the bulges of two interacting galaxies

Elkin L. López, Simon N. Kemp, Gustavo V. López

Two mathematical models of three bodies of variable masses are used to obtain a qualitative description of two interacting galaxies with mass exchange and mass loss. The reference…