Modeling the CO outflow in DG Tauri B: Swept-up shells versus perturbed MHD disk wind

0569257 - ASÚ 2023 RIV FR eng J - Journal Article
de Valon, A. … Total 6 authors
Modeling the CO outflow in DG Tauri B: Swept-up shells versus perturbed MHD disk wind.
Astronomy & Astrophysics. Roč. 668, December (2022), č. článku A78. ISSN 0004-6361. E-ISSN 1432-0746
Research Infrastructure: EU-ARC.CZ II - 90106
Keywords : stars formation * protostars * jets and outflows
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 6.5, year: 2022
Method of publishing: Open access
https://doi.org/10.1051/0004-6361/202141316

We aim to characterize the morphology and kinematics of the DG Tau B outflow in order to elucidate its origin and potential impact on the disk.
Permanent Link: https://hdl.handle.net/11104/0341270