activity
20142021
most citedA two-mode planetary nebula luminosity function

10 citations · 37 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2021

Velocity segregation in a clump-like outflow with a non-top hat velocity cross-section

A. Castellanos-Ramírez, A. C. Raga, J. Cantó +2

High velocity clumps joined to the outflow source by emission with a "Hubble law" ramp of linearly increasing radial velocity vs. distance are observed in some planetary nebulae an…

astro-ph.SR2021★ 3 cited

Twenty years of observations of PM 1-188: Its chemical abundances and extraordinary kinematics

Miriam Peña, Liliana Hernández-Martínez, Francisco Ruiz-Escobedo

The analysis of 20 years of spectrophotometric data of the double shell planetary nebula PM\,1-188 is presented, aiming to determine the time evolution of the emission lines and th…

astro-ph.GA2018★ 9 cited

Chemistry in the dIrr galaxy Leo A

Francisco Ruiz-Escobedo, Miriam Peña, Liliana Hernández-Martínez +1

We present chemical abundance determinations of two H II regions in the dIrr galaxy Leo A, from GTC OSIRIS long-slit spectra. Both H II regions are of low excitation and seem to be…

astro-ph.GA2016★ 9 cited

The metallic winds in dwarf galaxies

F. Robles-Valdez, A. Rodríguez-González, L. Hernández-Martínez +1

We present results from models of galactic winds driven by energy injected from nuclear (at the galactic center) and non-nuclear starbursts. The total energy of the starburst is pr…

astro-ph.GA2014★ 10 cited

A two-mode planetary nebula luminosity function

A. Rodríguez-González, L. Hernández-Martínez, A. Esquivel +4

We propose a new Planetary Nebula Luminosity Function (PNLF) that includes two populations in the distribution. Our PNLF is a direct extension of the canonical function proposed by…

astro-ph.GA2014★ 6 cited

Kinematic study of planetary nebulae in NGC 6822

S. N. Flores-Durán, M. Peña, L. Hernández-Martínez +2

By measuring precise radial velocities of planetary nebulae (which belong to the intermediate age population), H II regions, and A-type supergiant stars (which are members of the y…