activity
20092013
most citedQuadruple-peaked spectral line profiles as a tool to constrain gravitational potential of shell galaxies

30 citations · 71 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2013★ 22 cited

Testing MOND gravity in the shell galaxy NGC 3923

Michal Bilek, Bruno Jungwiert, Lucie Jilkova +3

Context. The elliptical galaxy NGC 3923 is surrounded by numerous stellar shells that are concentric arcs centered on the galactic core. They are very likely a result of a minor me…

astro-ph.CO2012★ 30 cited

Quadruple-peaked spectral line profiles as a tool to constrain gravitational potential of shell galaxies

Ivana Ebrova, Lucie Jilkova, Bruno Jungwiert +5

Stellar shells observed in many giant elliptical and lenticular as well as a few spiral and dwarf galaxies, presumably result from galaxy mergers. Line-of-sight velocity distributi…

astro-ph.GA2011

Comparing Various Approaches to Simulating the Formation of Shell Galaxies

Ivana Ebrova, Katerina Bartoskova, Bruno Jungwiert +2

The model of a radial minor merger proposed by Quinn (1984), which successfully reproduces the observed regular shell systems in shell galaxies, is ideal for a test-particle simula…

astro-ph.GA2011★ 3 cited

Quadruple-peaked Line-of-sight Velocity Distributions in Shell Galaxies

Ivana Ebrova, Lucie Jilkova, Bruno Jungwiert +4

We present an improved study of the expected shape of the line-of-sight velocity distribution in shell galaxies. We found a simple analytical expression connecting prominent and in…

astro-ph.GA2011★ 15 cited

Simulations of shell galaxies with GADGET-2: Multi-generation shell systems

Kateřina Bartošková, Bruno Jungwiert, Ivana Ebrová +2

As the missing complement to existing studies of shell galaxies, we carried out a set of self-consistent N-body simulations of a minor merger forming a stellar shell system within…

astro-ph.GA2009★ 1 cited

Simulations of Line Profile Structure in Shell Galaxies

L. Jilkova, B. Jungwiert, M. Krizek +4

In the context of exploring mass distributions of dark matter haloes in giant ellipticals, we extend the analysis carried out Merrifield and Kuijken (1998) for stellar line profile…