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Monthly Highlights

December 2020

Formation of pillar-like structures <br><i>by Sebastian Vider</i>

November 2020

Gravo turbulence or global hierarchical collapse? <br><i>by Shashwata Ganguly</i>

September 2020

Protostellar outflows increase the fraction of Twin-binaries <br><i>by Paul Rohde</i>

August 2020

Aluminum-26 Production in Protostellar Disks <br><i>by Brandt Gaches</i>

July 2020

Formation of Sink Particles using a subgrid model <br><i>by Timothy Crundall</i>

June 2020

Understanding synthetic polarization spectra <br><i>by Thorsten Balduin</i>

May 2020

Application of a novel radiative transfer scheme in the context of core collapse <br><i>by Andre Klepitko</i>

April 2020

Radiative feedback in molecular clouds from cooling supernova shock waves <br><i>by Ekaterina Makarenko</i>

March 2020

Binary stars in touch <br><i>by Dorottya Szécsi</i>

February 2020

Measuring the Star Formation Rate Across Epochs <br><i>by Thomas Bisbas</i>

January 2020

Fractional abundance of chemical species in 3D SPH simulations

December 2020

Formation of pillar-like structures <br><i>by Sebastian Vider</i>

November 2020

Gravo turbulence or global hierarchical collapse? <br><i>by Shashwata Ganguly</i>

September 2020

Protostellar outflows increase the fraction of Twin-binaries <br><i>by Paul Rohde</i>

August 2020

Aluminum-26 Production in Protostellar Disks <br><i>by Brandt Gaches</i>

July 2020

Formation of Sink Particles using a subgrid model <br><i>by Timothy Crundall</i>

June 2020

Understanding synthetic polarization spectra <br><i>by Thorsten Balduin</i>

May 2020

Application of a novel radiative transfer scheme in the context of core collapse <br><i>by Andre Klepitko</i>

April 2020

Radiative feedback in molecular clouds from cooling supernova shock waves <br><i>by Ekaterina Makarenko</i>

March 2020

Binary stars in touch <br><i>by Dorottya Szécsi</i>

February 2020

Measuring the Star Formation Rate Across Epochs <br><i>by Thomas Bisbas</i>

January 2020

Fractional abundance of chemical species in 3D SPH simulations