activity
20042025
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 5.8k across the 39 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

10 papers · 1 filter

astro-ph.CO2021★ 8 cited

Faint polarised sources in the Lockman Hole field at 1.4 GHz

A. Berger, B. Adebahr, N. Herrera Ruiz +3

We aim to study the nature of the faint, polarised radio source population whose source composition and redshift dependence contain information about the strength, morphology, and…

astro-ph.CO2011★ 1.3k cited

CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

S. F. Sanchez, R. C. Kennicutt, A. Gil de Paz +69

We present here the Calar Alto Legacy Integral Field Area (CALIFA) survey, which has been designed to provide a first step in this direction.We summarize the survey goals and desig…

astro-ph.CO2011★ 21 cited

Hot gas in Mach cones around Virgo Cluster spiral galaxies

M. Wezgowiec, B. Vollmer, M. Ehle +5

The detailed comparison between observations and simulations of ram pressure stripped spiral galaxies in the Virgo cluster has led to a three dimensional view of the galaxy orbits…

astro-ph.CO2011★ 50 cited

Lopsidedness in WHISP galaxies: II. Morphological lopsidedness

J. van Eymeren, E. Juette, C. J. Jog +2

The distribution of stars and gas in many galaxies is asymmetric. This so-called lopsidedness is expected to significantly affect the dynamics and evolution of the disc, including…

astro-ph.CO2011★ 43 cited

Lopsidedness in WHISP galaxies: I. Rotation curves and kinematic lopsidedness

J. van Eymeren, E. Juette, C. J. Jog +2

The frequently observed lopsidedness of the distribution of stars and gas in disc galaxies is still considered as a major problem in galaxy dynamics. It is even discussed as an imp…

astro-ph.CO2010

Lopsidedness in WHISP galaxies

Eva Juette, Janine van Eymeren, Chanda Jog +2

Observations of the stellar and gaseous components in disc galaxies often reveal asymmetries in the morphological and kinematic distribution. However, the origin of this effect is…

astro-ph.CO2009★ 8 cited

Transport of cosmic rays in the nearby starburst galaxy NGC 253

Volker Heesen, Rainer Beck, Marita Krause +1

Radio halos require the coexistence of extra-planar cosmic rays and magnetic fields. Because cosmic rays are injected and accelerated by processes related to star formation in the…

astro-ph.CO2009★ 111 cited

The baryonic Tully-Fisher relation and its implication for dark matter halos

C. Trachternach, W. J. G. de Blok, S. S. McGaugh +2

The baryonic Tully-Fisher relation (BTF) is a fundamental relation between baryonic mass and maximum rotation velocity. It can be used to estimate distances, as well as to constrai…

astro-ph.CO2009★ 23 cited

The age of blue LSB galaxies

E. I. Vorobyov, Yu. Shchekinov, D. Bizyaev +3

(Abridged). Low metallicities, large gas-to-star mass ratios, and blue colors of most low surface brightness (LSB) galaxies imply that these systems may be younger than their high…

astro-ph.CO2009★ 34 cited

Non-circular motions and the cusp-core discrepancy in dwarf galaxies

J. van Eymeren, C. Trachternach, B. S. Koribalski +1

Context. The cusp-core discrepancy is one of the major problems in astrophysics. It results from comparing the observed mass distribution of galaxies with the predictions of Cold D…