Early evolution of viscous and self-gravitating circumstellar disks with a dust component › Research Explorer

Novosibirsk State University's Research Portal

Early evolution of viscous and self-gravitating circumstellar disks with a dust component

Research output: Contribution to journal › Article › peer-review

Energy-Saving Catalytic Processes Laboratory

DOI

https://doi.org/10.1051/0004-6361/201731690
Final published version

Eduard I. Vorobyov
Vitaly Akimkin
Olga Stoyanovskaya
Yaroslav Pavlyuchenkov
Hauyu Baobab Liu

Original language	English
Article number	A98
Number of pages	20
Journal	Astronomy and Astrophysics
Volume	614
DOIs	https://doi.org/10.1051/0004-6361/201731690
Publication status	Published - 21 Jun 2018

OECD FOS+WOS

Research areas

Hydrodynamics, Protoplanetary disks, Stars: formation, Stars: protostars, PROTOSTELLAR ACCRETION, stars: protostars, CONTINUUM OBSERVATIONS, GIANT PLANETS, FU ORIONIS, BURST MODE, hydrodynamics, stars: formation, GROWTH, GAS, PLANETESIMAL FORMATION, ELECTROSTATIC BARRIER, protoplanetary disks, RESOLUTION (CO)-O-18

ID: 14403949