activity
19972019
most citedThe Mass-Metallicity relation explored with CALIFA: I. Is there a dependence on the star formation rate?

276 citations · 1.9k across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.GA2019★ 3 cited

Utilizing Shell Galaxies

Ivana Ebrová, Michal Bílek, Bruno Jungwiert

Stellar shells are low surface brightness features in the form of open, concentric arcs, formed in close-to-radial collisions of galaxies. They occur in at least 10% of early-type…

astro-ph.GA2015★ 28 cited

Deep imaging of the shell elliptical galaxy NGC3923 with MegaCam

Michal Bílek, Jean-Charles Cuillandre, Stephen Gwyn +4

Context. The elliptical galaxy NGC 3923 is known to be surrounded by a number of stellar shells, probable remnants of an accreted galaxy. Despite its uniqueness, the deepest images…

astro-ph.GA2015★ 6 cited

MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations

Michal Bílek, Bruno Jungwiert, Ivana Ebrová +1

Context. Many ellipticals are surrounded by round stellar shells probably stemming from minor mergers. A new method for constraining gravitational potential in elliptical galaxies…

astro-ph.GA2014★ 240 cited

CALIFA, the Calar Alto Legacy Integral Field Area survey. III. Second public data release

R. García-Benito, S. Zibetti, S. F. Sánchez +68

This paper describes the Second Public Data Release (DR2) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. The data for 200 objects are made public, including the 100…

astro-ph.GA2014★ 15 cited

Shell galaxies as laboratories for testing MOND

Michal Bílek, Ivana Ebrová, Bruno Jungwiert +2

Tests of MOND in ellipticals are relatively rare because these galaxies often lack kinematic tracers in the regions where the MOND effects are significant. Stellar shells observed…

astro-ph.GA2014★ 207 cited

Stellar Population gradients in galaxy discs from the CALIFA survey

P. Sanchez-Blazquez, F. Rosales-Ortega, J. Mendez-Abreu +27

While studies of gas-phase metallicity gradients in disc galaxies are common, very little has been done in the acquisition of stellar abundance gradients in the same regions. We pr…