activity
20142020
most citedRadiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields

108 citations · 171 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2020108 cited

Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields

Sylvia Ploeckinger, Joop Schaye

We use the spectral synthesis code Cloudy to tabulate the properties of gas for an extensive range in redshift (z=0 to 9), temperature (log T [K] = 1 to 9.5), metallicity (log Z/$\…

astro-ph.GA201911 cited

Abundance and group coalescence timescales of compact groups of galaxies in the EAGLE simulation

Len Hartsuiker, Sylvia Ploeckinger

Observations of compact groups of galaxies (CGs) indicate that their abundance has not significantly changed since . This balance between the timescales for formation and de…

astro-ph.GA20195 cited

Does radiative feedback make faint z>6 galaxies look small?

Sylvia Ploeckinger, Joop Schaye, Alvaro Hacar +3

Recent observations of lensed sources have shown that the faintest () galaxies observed at z=6-8 appear to be extremely compact. Some of…

astro-ph.GA201447 cited

Chemo-dynamical evolution of tidal dwarf galaxies. II. The long-term evolution and influence of a tidal field

Sylvia Ploeckinger, Simone Recchi, Gerhard Hensler +1

In a series of papers, we present detailed chemo-dynamical simulations of tidal dwarf galaxies (TDGs). After the first paper, where we focused on the very early evolution, we prese…

astro-ph.GA2014

Simulations on the survivability of Tidal Dwarf Galaxies

Sylvia Ploeckinger, Simone Recchi, Gerhard Hensler +1

We present detailed numerical simulations of the evolution of Tidal Dwarf Galaxies (TDGs) after they kinematically decouple from the rest of the tidal arm to investigate their surv…