Stringent limits on the magnetic field strength in the disc of TW Hya: ALMA observations of CN polarisation
Artikel i vetenskaplig tidskrift, 2019
Despite their importance in the star formation process, measurements of magnetic field strength in proto-planetary discs remain rare. While linear polarisation of dust and molecular lines can give insight into the magnetic field structure, only observations of the circular polarisation produced by Zeeman splitting provide a direct measurement of magnetic field strenghts. One of the most promising probes of magnetic field strengths is the paramagnetic radical CN. Here we present the first Atacama Large Millimeter/submillimeter Array (ALMA) observations of the Zeeman splitting of CN in the disc of TW Hya. The observations indicate an excellent polarisation performance of ALMA, but fail to detect significant polarisation. An analysis of eight individual CN hyperfine components as well as a stacking analysis of the strongest (non-blended) hyperfine components yields the most stringent limits obtained so far on the magnetic field strength in a proto-planetary disc. We find that the vertical component of the magnetic field vertical bar B-z vertical bar < 0.8 mG (1 sigma limit). We also provide a 1 sigma toroidal field strength limit of < 30 mG. These limits rule out some of the earlier accretion disc models, but remain consistent with the most recent detailed models with e ffi cient advection. We detect marginal linear polarisation from the dust continuum, but the almost purely toroidal geometry of the polarisation vectors implies that his is due to radiatively aligned grains.
magnetic fields
stars: individual: TW Hya
accretion, accretion disks
stars: pre-main sequence
Författare
Wouter Vlemmings
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Boy Lankhaar
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
P. Cazzoletti
Max-Planck-Gesellschaft
Chiara Ceccobello
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Daria Dall` Olio
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
E. F. van Dishoeck
Max-Planck-Gesellschaft
Universiteit Leiden
S. Facchini
European Southern Observatory Santiago
E. M. L. Humphreys
European Southern Observatory Santiago
Magnus V. Persson
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
L. Testi
European Southern Observatory Santiago
Osservatorio Astrofisico di Arcetri
Ludwig-Maximilians-Universität München (LMU)
J. P. Williams
University of Hawaii
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 624 L7Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/201935459