activity
20142023
most citedKinematic clues to bar evolution for galaxies in the local universe: why the fastest rotating bars are rotating most slowly

47 citations · 88 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20238 cited

Measuring the physical imprints of gas flows in galaxies I: Accretion rate histories

A. Camps-Fariña, P. Sánchez-Blázquez, S. Roca-Fàbrega +1

Galaxies are expected to accrete pristine gas from their surroundings to sustain their star formation over cosmic timescales. Its lower abundance affects the metallicity of the ISM…

astro-ph.HE202217 cited

Rectangular core-collapse supernova remnants: application to Puppis A

D. M. -A. Meyer, P. F. Velazquez, O. Petruk +9

Core-collapse supernova remnants are the gaseous nebulae of galactic interstellar media (ISM) formed after the explosive death of massive stars. Their morphology and emission prope…

astro-ph.GA201747 cited

Kinematic clues to bar evolution for galaxies in the local universe: why the fastest rotating bars are rotating most slowly

J. Font, J. E. Beckman, I. Martínez-Valpuesta +7

We have used Spitzer images of a sample of 68 barred spiral galaxies in the local universe to make systematic measurements of bar length and bar strength. We combine these with pre…

astro-ph.GA20167 cited

Kinematics of the ionized and molecular gas in nearby luminous infrared interacting galaxies

Javier Zaragoza-Cardiel, John Beckman, Joan Font +3

We have observed three luminous infrared galaxy systems (LIRGS) which are pairs of interacting galaxies, with the Galaxy H Fabry-Perot system (GHFaS) mounted on the 4.2m Will…

astro-ph.IM20149 cited

BUBBLY: A method for detecting and characterizing interstellar bubbles using Fabry-Perot spectroscopy

Artemi Camps-Fariña, Javier Zaragoza-Cardiel, John E. Beckman +4

We present a new method for the detection and characterization of expansion in galaxy discs based on Hα Fabry-Perot spectroscopy, taking advantage of the high spatial and velocity…