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Chemical Evolution of Turbulent Protoplanetary Disks and the Solar Nebula

The Astrophysical journal. Supplement series, 2011-10, Vol.196 (2), p.25-jQuery1323919630395='48'

2011

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Dust dynamics and evolution in expanding H ii regions. I. Radiative drift of neutral and charged grains

Monthly notices of the Royal Astronomical Society, 2015-05, Vol.449 (1), p.440-450

2015

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Objectives of the Millimetron Space Observatory science program and technical capabilities of its realization

Physics Uspekhi, , Vol.64 (4), p.386-419

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Efficiency of the top-down polycyclic aromatic hydrocarbon-to-fullerene conversion in ultraviolet irradiated environments

Monthly notices of the Royal Astronomical Society, 2022-10, Vol.517 (3), p.3732-3748

2022

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Improved Constraints on Cosmology and Foregrounds from BICEP2 and Keck Array Cosmic Microwave Background Data with Inclusion of 95 GHz Band

Physical review letters, 2016-01, Vol.116 (3), p.031302-031302, Article 031302

2016

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shiva: a dust destruction model

Monthly notices of the Royal Astronomical Society, 2019-09, Vol.488 (1), p.965-977

2019

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PROTOPLANETARY DISK STRUCTURE WITH GRAIN EVOLUTION: THE ANDES MODEL

The Astrophysical journal, 2013-03, Vol.766 (1), p.1-24

2013

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Molecular and Atomic Gas in Star-forming Complexes: NGC 5194, NGC 5457, NGC 628, and NGC 6946

Astronomy reports, 2022-04, Vol.66 (4), p.330-340

2022

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Star formation time-scale in the molecular filament WB 673

Monthly notices of the Royal Astronomical Society, 2022-11, Vol.517 (4), p.4669-4678

2022

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BICEP2 / Keck Array IX: New bounds on anisotropies of CMB polarization rotation and implications for axionlike particles and primordial magnetic fields

Physical review. D, 2017-11, Vol.96 (10), Article 102003

2017

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Limits on the Ultra-bright Fast Radio Burst Population from the CHIME Pathfinder

The Astrophysical journal, 2017-08, Vol.844 (2), p.161

2017

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Polycyclic aromatic hydrocarbons in spatially resolved extragalactic star-forming complexes

Monthly notices of the Royal Astronomical Society, 2013-05, Vol.431 (2), p.2006-2016

2013

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Physical conditions in star-forming regions around S235

Monthly notices of the Royal Astronomical Society, 2014-01, Vol.437 (2), p.1593-1608

2014

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Review of scientific topics for the Millimetron space observatory

Physics Uspekhi, 2014-01, Vol.57 (12), p.1199-1228

2014

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The warm-up phase in massive star-forming cores around RCW 120

Monthly notices of the Royal Astronomical Society, 2021-03, Vol.503 (1), p.633-642

2021

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Molecular envelope around the HII region RCW 120

Monthly notices of the Royal Astronomical Society, 2019-10, Vol.488 (4), p.5641-5650

2019

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Observations in the UV Band and Problems of Star Formation Studies

Solar system research, 2017-12, Vol.51 (7), p.587-591

Wiebe, D. S.

2017

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Optical and infrared emission of H ii complexes as a clue to the PAH life cycle

Monthly notices of the Royal Astronomical Society, 2014-10, Vol.444 (1), p.757-775

2014

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A Unified Monte Carlo Treatment of Gas-Grain Chemistry for Large Reaction Networks. I. Testing Validity of Rate Equations in Molecular Clouds

The Astrophysical journal, 2009-02, Vol.691 (2), p.1459-1469

2009

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Gas-Phase CO in Protoplanetary Disks: A Challenge for Turbulent Mixing

The Astrophysical journal, 2006-08, Vol.647 (1), p.L57-L60

2006

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The Balloon-borne Large Aperture Submillimeter Telescope: BLAST

The Astrophysical journal, 2008-07, Vol.681 (1), p.400-414

2008

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Uncertainty in Estimates of Dissociation Rates of Polycyclic Aromatic Hydrocarbons in the Interstellar Medium

Bulletin of the Lebedev Physics Institute, 2022-12, Vol.49 (12), p.416-421

2022

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Infrared emission and the destruction of dust in HII regions

Astronomy reports, 2013-08, Vol.57 (8), p.573-585

2013

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A New Modified-Rate Approach For Gas-Grain Chemistry: Comparison with a Unified Large-Scale Monte Carlo Simulation

The Astrophysical journal, 2009-07, Vol.700 (1), p.L43-L46

2009

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Deuterated Isotopologues of Water and Methanol in Star-Forming Regions

Astronomy letters, 2020-06, Vol.46 (6), p.379-387

2020

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Chemical Evolution of Turbulent Protoplanetary Disks and the Solar Nebula

Dust dynamics and evolution in expanding H ii regions. I. Radiative drift of neutral and charged grains

Objectives of the Millimetron Space Observatory science program and technical capabilities of its realization

Efficiency of the top-down polycyclic aromatic hydrocarbon-to-fullerene conversion in ultraviolet irradiated environments

Improved Constraints on Cosmology and Foregrounds from BICEP2 and Keck Array Cosmic Microwave Background Data with Inclusion of 95 GHz Band

shiva: a dust destruction model

PROTOPLANETARY DISK STRUCTURE WITH GRAIN EVOLUTION: THE ANDES MODEL

Molecular and Atomic Gas in Star-forming Complexes: NGC 5194, NGC 5457, NGC 628, and NGC 6946

Star formation time-scale in the molecular filament WB 673

BICEP2 / Keck Array IX: New bounds on anisotropies of CMB polarization rotation and implications for axionlike particles and primordial magnetic fields

Limits on the Ultra-bright Fast Radio Burst Population from the CHIME Pathfinder

Polycyclic aromatic hydrocarbons in spatially resolved extragalactic star-forming complexes

Physical conditions in star-forming regions around S235

Review of scientific topics for the Millimetron space observatory

The warm-up phase in massive star-forming cores around RCW 120

Molecular envelope around the HII region RCW 120

Observations in the UV Band and Problems of Star Formation Studies

Optical and infrared emission of H ii complexes as a clue to the PAH life cycle

A Unified Monte Carlo Treatment of Gas-Grain Chemistry for Large Reaction Networks. I. Testing Validity of Rate Equations in Molecular Clouds

Gas-Phase CO in Protoplanetary Disks: A Challenge for Turbulent Mixing

The Balloon-borne Large Aperture Submillimeter Telescope: BLAST

Uncertainty in Estimates of Dissociation Rates of Polycyclic Aromatic Hydrocarbons in the Interstellar Medium

Infrared emission and the destruction of dust in HII regions

A New Modified-Rate Approach For Gas-Grain Chemistry: Comparison with a Unified Large-Scale Monte Carlo Simulation

Deuterated Isotopologues of Water and Methanol in Star-Forming Regions

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