output
19942026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations

Showing 2016Show all

38 papers · 1 filter

astro-ph.SR2016★ 166 cited

Structure of Herbig AeBe disks at the milliarcsecond scale A statistical survey in the H band using PIONIER-VLTI

B. Lazareff, J. -P. Berger, J. Kluska +26

Context. It is now generally accepted that the near-infrared excess of Herbig AeBe stars originates in the dust of a circumstellar disk. Aims. The aims of this article are to infer…

astro-ph.GA2016★ 127 cited

High-redshift major mergers weakly enhance star formation

J. Fensch, F. Renaud, F. Bournaud +11

Galaxy mergers are believed to trigger strong starbursts. This is well assessed by observations in the local Universe. However the efficiency of this mechanism has poorly been test…

astro-ph.GA2016★ 31 cited

Ly Emitters with Very Large Ly Equivalent Widths, EW(Ly) Å, at

Takuya Hashimoto, Masami Ouchi, Kazuhiro Shimasaku +6

We present physical properties of spectroscopically confirmed Ly emitters (LAEs) with very large rest-frame Ly equivalent widths EW(Ly). Although the definition…

astro-ph.GA2016★ 90 cited

SDSS-IV MaNGA: Properties of galaxies with kinematically decoupled stellar and gaseous components

Yifei Jin, Yanmei Chen, Yong Shi +30

We study the properties of 66 galaxies with kinematically misaligned gas and stars from MaNGA survey. The fraction of kinematically misaligned galaxies varies with galaxy physical…

astro-ph.GA2016★ 53 cited

The growth of the central region by acquisition of counter-rotating gas in star-forming galaxies

Yan-Mei Chen, Yong Shi, Christy A. Tremonti +29

Galaxies grow through both internal and external processes. In about 10% of nearby red galaxies with little star formation, gas and stars are counter-rotating, demonstrating the im…

astro-ph.GA2016★ 145 cited

Density profile of dark matter haloes and galaxies in the Horizon-AGN simulation: the impact of AGN feedback

S. Peirani, Y. Dubois, M. Volonteri +7

Using a suite of three large cosmological hydrodynamical simulations, Horizon-AGN, Horizon-noAGN (no AGN feedback) and Horizon-DM (no baryons), we investigate how a typical sub-gri…