Space Chemical Reactor of Protoplanetary Disk
Full article
| Common |
Language:
Английский,
Genre:
Full article,
Status:
Published,
Source type:
Original
|
| Conference |
33rd COSPAR Scientific Assembly
16-23 Jul 2000
,
Warsaw
|
| Journal |
Advances in Space Research
ISSN: 0273-1177
|
| Output data |
Year: 2002,
Volume: 30,
Number: 6,
Pages: 1461-1467
Pages count
: 7
DOI:
10.1016/S0273-1177(02)00507-0
|
| Authors |
Snytnikov V.N.
1
,
Dudnikova G.I.
2
,
Gleaves J.T.
3
,
Nikitin S.A.
4
,
Parmon V.N.
1
,
Stoyanovsky V.O.
1
,
Vshivkov V.A.
2
,
Yablonsky G.S.
3
,
Zakharenko V.S.
1
|
| Affiliations |
| 1 |
Boreskov Institute of Catalysis, Prospect Lavrentieva, 5, Novosibirsk 630090, Russia
|
| 2 |
Institute of Computational Technology, Novosibirsk, Russia
|
| 3 |
Washington University, St. Louis, MO 63130, USA
|
| 4 |
Budker Institute of Nuclear Physics, Novosibirsk, Russia
|
|
It was found that the protostar accretion disk is the place of organic compounds synthesis from simple molecules. The mass of the matter moving around the synthesis zone is comparable to the solar mass. The formed amount of organic substance may be limited by the instability of collective dynamics of solids in the disk.