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

collaborators
Showing 2020Show all

5 papers · 1 filter

astro-ph.HE2020★ 27 cited

Evolution and observational signatures of the cosmic ray electron spectrum in SN 1006

Georg Winner, Christoph Pfrommer, Philipp Girichidis +2

Supernova remnants (SNRs) are believed to be the source of Galactic cosmic rays (CRs). SNR shocks accelerate CR protons and electrons which reveal key insights into the non-thermal…

astro-ph.GA2020★ 127 cited

The Physics of Star Cluster Formation and Evolution

Martin G. H. Krause, Stella S. R. Offner, Corinne Charbonnel +8

Star clusters form in dense, hierarchically collapsing gas clouds. Bulk kinetic energy is transformed to turbulence with stars forming from cores fed by filaments. In the most comp…

astro-ph.GA2020★ 80 cited

Physical Processes in Star Formation

Philipp Girichidis, Stella S. R. Offner, Alexei G. Kritsuk +6

Star formation is a complex multi-scale phenomenon that is of significant importance for astrophysics in general. Stars and star formation are key pillars in observational astronom…

astro-ph.GA2020★ 123 cited

Impact of low-energy cosmic rays on star formation

Marco Padovani, Alexei V. Ivlev, Daniele Galli +7

In recent years, exciting developments have taken place in the identification of the role of cosmic rays in star-forming environments. Observations from radio to infrared wavelengt…

astro-ph.GA2020

Statistical mass function of prestellar cores from the density distribution of their natal clouds

S. Donkov, T. V. Veltchev, Ph. Girichidis +1

The mass function of clumps observed in molecular clouds raises interesting theoretical issues, especially in its relation to the stellar initial mass function. We propose a statis…