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

0569257 - ASÚ 2023 RIV FR eng J - Článek v odborném periodiku
de Valon, A. … celkem 6 autorů
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
Výzkumná infrastruktura: EU-ARC.CZ II - 90106
Klíčová slova: stars formation * protostars * jets and outflows
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 6.5, rok: 2022
Způsob publikování: 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.
Trvalý link: https://hdl.handle.net/11104/0341270