activity
20102026
most citedThe SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM

367 citations · 3.9k across the 78 of their papers we have counts for

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Showing 2018Show all

6 papers · 1 filter

astro-ph.GA2018★ 38 cited

Synthetic [CII] emission maps of a simulated molecular cloud in formation

A. Franeck, S. Walch, D. Seifried +10

The C ion is an important coolant of interstellar gas, and so the [CII] fine structure line is frequently observed in the interstellar medium. However, the physical and chemi…

astro-ph.GA2018★ 69 cited

The SILCC project - V. The impact of magnetic fields on the chemistry and the formation of molecular clouds

Philipp Girichidis, Daniel Seifried, Thorsten Naab +5

Magnetic fields are ubiquitously observed in the interstellar medium (ISM) of present-day star-forming galaxies with dynamically relevant energy densities. Using three-dimensional…

astro-ph.GA2018★ 152 cited

Cooler and smoother -- the impact of cosmic rays on the phase structure of galactic outflows

Philipp Girichidis, Thorsten Naab, Michał Hanasz +1

We investigate the impact of cosmic rays (CRs) on galactic outflows from a multi-phase interstellar medium with solar neighbourhood conditions. The three-dimensional magneto-hydrod…

astro-ph.GA2018★ 22 cited

The imprint of cosmic ray driven outflow on Lyman-alpha spectra

Max Gronke, Philipp Girichidis, Thorsten Naab +1

Recent magneto-hydrodynamic simulations of the star-forming interstellar medium (ISM) with parsec scale resolution indicate that relativistic cosmic rays support the launching of g…

astro-ph.GA2018★ 48 cited

Is molecular cloud turbulence driven by external supernova explosions?

D. Seifried, S. Walch, S. Haid +2

We present high-resolution ( 0.1 pc), hydrodynamical and magnetohydrodynamical simulations to investigate whether the observed level of molecular cloud (MC) turbulence can be…

astro-ph.GA2018★ 28 cited

Radiative transfer calculations of the diffuse ionised gas in disc galaxies with cosmic ray feedback

Bert Vandenbroucke, Kenneth Wood, Philipp Girichidis +2

The large vertical scale heights of the diffuse ionised gas (DIG) in disc galaxies are challenging to model, as hydrodynamical models including only thermal feedback seem to be una…