Can we Expect the Massive Disc Around Young Stellar Object Class O/I to be a Birthplace of Planetesimal Formation? | Sciact - CRIS-system of Boreskov Institute of Catalysis

Can we Expect the Massive Disc Around Young Stellar Object Class O/I to be a Birthplace of Planetesimal Formation? Conference Abstracts

Conference

IAU-Symposium: Complex Planetary Systems
07-11 Jul 2014 , Namur

Source

IAU-Symposium: Complex Planetary Systems
Compilation, 2014.

Output data

Year: 2014, Pages: F10 Pages count : 1

Authors

Stoyanovskaya O.P. , Snytnikov V.N. , Stadnichenko O.A.

Affiliations

1	Boreskov Institute of Catalysis SB RAS
2	Novosibirsk National Research University

Stoyanovskaya O.P. , Snytnikov V.N. , Stadnichenko O.A.
Can we Expect the Massive Disc Around Young Stellar Object Class O/I to be a Birthplace of Planetesimal Formation?
In compilation IAU-Symposium: Complex Planetary Systems. 2014. – C.F10.

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