Dmitry Semenov
www.mpia.de
0000-0002-3913-7114
130 papers found
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Modeling the NIR-silhouette massive disk candidate in M 17
Gas-Phase CO in Protoplanetary Disks: A Challenge for Turbulent Mixing
A Rotating Disk around the Very Young Massive Star AFGL 490
Millimeter Observations and Modeling of the AB Aurigae System
Chemistry of Ionization in Evolving Disks
Importance of turbulent mixing and advective transport for the chemical evolution of protoplanetary disks
Millimeter observations and modeling of the AB Aur system
The massive disk around the young B-star AFGL 490
Modeling the NIR-Silhouette Massive Disk Candidate in M17
Chemistry of Ionization
Influence of uncertainties in the rate constants of chemical reactions on astrochemical modeling results
On the Feasibility of Chemical Modeling of a Proplanetary Disk
Reduction of chemical networks. II. Analysis of the fractional ionisation in protoplanetary discs
Ionization Structure of Protoplanetary Disks from the Chemical Perspective
Rosseland and Planck mean opacities for protoplanetary discs
On the Feasibility of Disk Chemical Modeling
A database of optical constants of cosmic dust analogs
3D continuum radiative transfer in complex dust configurations around stellar objects and active galactic nuclei. I. Computational methods and capabilities
Chemistry in Star-Forming Regions: Making Complex Modelling Feasible
Metamorphosis of a BD Disk: Flared Becomes Flat
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