ALMA discovery of a rotating SO/SO2 flow in HH212

We wish to constrain the possible contribution of a magnetohydrodynamic disk wind (DW) to the HH212 molecular jet. We mapped the flow base with ALMA Cycle 4 at 0.̋13 ~ 60 au resolution and compared these observations with synthetic DW predictions. We identified, in SO/SO2, a rotating flow that is wi...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2017-11, Vol.607
Hauptverfasser: Tabone, B., Cabrit, S., Bianchi, E., Ferreira, J., Pineau des Forêts, G., Codella, C., Gusdorf, A., Gueth, F., Podio, L., Chapillon, E.
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container_title Astronomy and astrophysics (Berlin)
container_volume 607
creator Tabone, B.
Cabrit, S.
Bianchi, E.
Ferreira, J.
Pineau des Forêts, G.
Codella, C.
Gusdorf, A.
Gueth, F.
Podio, L.
Chapillon, E.
description We wish to constrain the possible contribution of a magnetohydrodynamic disk wind (DW) to the HH212 molecular jet. We mapped the flow base with ALMA Cycle 4 at 0.̋13 ~ 60 au resolution and compared these observations with synthetic DW predictions. We identified, in SO/SO2, a rotating flow that is wider and slower than the axial SiO jet. The broad outflow cavity seen in C34S is not carved by a fast wide-angle wind but by this slower agent. Rotation signatures may be fitted by a DW of a moderate lever arm launched out to ~40 au with SiO tracing dust-free streamlines from 0.05−0.3 au. Such a DW could limit the core-to-star efficiency to ≤50%.
doi_str_mv 10.1051/0004-6361/201731691
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subjects Flow mapping
Fluid dynamics
Fluid flow
ISM: individual objects: HH212
ISM: jets and outflows
Magnetohydrodynamics
Molecular chains
Outflow
Rotation
stars: formation
Stellar winds
Sulfur dioxide
title ALMA discovery of a rotating SO/SO2 flow in HH212
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