Dmitry Semenov
www.mpia.de
0000-0002-3913-7114
130 papers found
Refreshing results…
The chemical evolution in the early phases of massive star formation
Resolving the Chemical Substructure of Orion-KL
Protoplanetary Disk Structure With Grain Evolution: The Andes Model
Deuterium fractionation of water in the Solar nebula
Molecular imprint of dust evolution
Chemistry in disks
Chemistry in Disks. Vii. First Detection of Hc3n in Protoplanetary Disks
Modeling deuterium chemistry of interstellar space with large chemical networks
Chemistry in protoplanetary disks
Tracing the evolutionary stage of Bok globules: CCS and NH3
Chemical Evolution of Turbulent Protoplanetary Disks and the Solar Nebula
Chemical Evolution of a Protoplanetary Disk
Deuterium chemistry in protoplanetary disks
CHEMISTRY OF a PROTOPLANETARY DISK WITH GRAIN SETTLING AND Lyα RADIATION
CHEMISTRY IN DISKS. III. PHOTOCHEMISTRY AND X-Ray DRIVEN CHEMISTRY PROBED BY THE ETHYNYL RADICAL (CCH) IN DM Tau, LkCa 15, AND MWC 480
Chemical and Isotopic Evolution of the Solar Nebula and Protoplanetary Disks
A New Modified-Rate Approach for Gas-Grain Chemistry: Comparison With a Unified Large-Scale Monte Carlo Simulation
A Unified Monte Carlo Treatment of Gas-Grain Chemistry for Large Reaction Networks. I. Testing Validity of Rate Equations in Molecular Clouds
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