Dmitry Semenov
www.mpia.de
0000-0002-3913-7114
130 papers found
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Gas Mass Tracers in Protoplanetary Disks: CO is Still the Best
The Flying Saucer: Tomography of the thermal and density gas structure of an edge-on protoplanetary disk
Origin of the RNA world: The fate of nucleobases in warm little ponds
Efficiency of thermal relaxation by radiative processes in protoplanetary discs: constraints on hydrodynamic turbulence
The chemical structure of the Class 0 protostellar envelope NGC 1333 IRAS 4A
Magnetic diffusivities in 3D radiative chemo-hydrodynamic simulations of protostellar collapse
On the methanol emission detection in the TW Hya disc: the role of grain surface chemistry and non-LTE excitation
A Surface Density Perturbation in the TW Hydrae Disk at 95 au Traced by Molecular Emission
Grain Surface Models and Data for Astrochemistry
The chemical structure of the Class 0 protostellar envelope NGC 1333 IRAS 4A⋆$\lt$/xref$\gt$⋆
ALCHEMIC: Advanced time-dependent chemical kinetics
Importance of the H2abundance in protoplanetary disk ices for the molecular layer chemical composition
Inferring the evolutionary stages of the internal structures of NGC 7538 S and IRS1 from chemistry
Chemistry in disks
Measuring turbulence in TW Hydrae with ALMA: methods and limitations
VizieR Online Data Catalog: TW Hya CO (2-1), CN (2-1) and CS (5-4) data cubes (Teague+, 2016)
Towards detecting methanol emission in low-mass protoplanetary discs with ALMA: the role of non-LTE excitation
Resolving the chemical substructure of Orion-KL(Corrigendum)
Cold Co Gas in the Disk of the Young Eruptive Star Ex Lup
The shadow of the Flying Saucer: A very low temperature for large dust grains
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