478 citations · 20.2k across the 337 of their papers we have counts for
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Exploring the nature of the Lyman- emitter CR7
Tilman Hartwig, Muhammad A. Latif, Mattis Magg +6
CR7 is the brightest Lyman- emitter observed at , which shows very strong Lyman- and HeII 1640Å line luminosities, but no metal line emission. Previous studies suggest t…
Hunting for the signatures of molecular cloud formation
Simon C. O. Glover, Paul C. Clark
In order to understand how molecular clouds form in the Galactic interstellar medium, we would like to be able to map the structure and kinematics of the gas flows responsible for…
Impact of supernova and cosmic-ray driving on the surface brightness of the galactic halo in soft X-rays
Thomas Peters, Philipp Girichidis, Andrea Gatto +7
The halo of the Milky Way contains a hot plasma with a surface brightness in soft X-rays of the order erg cm s deg. The origin of this gas is unclear…
Star formation and molecular hydrogen in dwarf galaxies: a non-equilibrium view
Chia-Yu Hu, Thorsten Naab, Stefanie Walch +2
We study the connection of star formation to atomic (HI) and molecular hydrogen (H) in isolated, low metallicity dwarf galaxies with high-resolution ( = 4 M$_\odot…
On the nature of star-forming filaments: II. Sub-filaments and velocities
Rowan J. Smith, Simon C. O. Glover, Ralf S. Klessen +1
We show that hydrodynamic turbulent cloud simulations naturally produce large filaments made up of a network of smaller and coherent sub-filaments. Such simulations resemble observ…
Launching cosmic-ray-driven outflows from the magnetized interstellar medium
Philipp Girichidis, Thorsten Naab, Stefanie Walch +10
We present a hydrodynamical simulation of the turbulent, magnetized, supernova (SN)-driven interstellar medium (ISM) in a stratified box that dynamically couples the injection and…