Studying stellar spin-down with Zeeman–Doppler magnetograms

See, V. and Jardine, M. and Vidotto, A. A. and Donati, J-F. and Boro Saikia, S. and Fares, R. and Folsom, C. P. and Hebrard, E. M. and Jeffers, S. V. and Marsden, S. C. and Morin, J. and Petit, P. and Waite, I. A. and BCool Collaboration, (2017) Studying stellar spin-down with Zeeman–Doppler magnetograms. Monthly Notices of the Royal Astronomical Society, 466 (2). pp. 1542-1554. ISSN 0035-8711

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Abstract

Magnetic activity and rotation are known to be intimately linked for low-mass stars. Understanding rotation evolution over the stellar lifetime is therefore an important goal within stellar astrophysics. In recent years, there has been increased focus on how the complexity of the stellar magnetic field affects the rate of angular-momentum loss from a star. This is a topic that Zeeman–Doppler imaging (ZDI), a technique that is capable of reconstructing the large-scale magnetic field topology of a star, can uniquely address. Using a potential field source surface model, we estimate the open flux, mass-loss rate and angular-momentum-loss rates for a sample of 66 stars that have been mapped with ZDI. We show that the open flux of a star is predominantly determined by the dipolar component of its magnetic field for our choice of source surface radius. We also show that, on the main sequence, the open flux, mass loss and angular-momentum-loss rates increase with decreasing Rossby number. The exception to this rule is stars less massive than 0.3Msun. Previous work suggests that low-mass M dwarfs may possess either strong, ordered and dipolar fields or weak and complex fields. This range of field strengths results in a large spread of angular momentum-loss rates for these stars and has important consequences for their spin-down behaviour. Additionally, our models do not predict a transition in the mass-loss rates at the so-called wind-dividing line noted from Lyα studies.


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Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Additional Information: Access to Published version in accordance with the copyright policy of the publisher.
Faculty / Department / School: Current - Faculty of Health, Engineering and Sciences - School of Agricultural, Computational and Environmental Sciences
Date Deposited: 19 Jan 2018 06:20
Last Modified: 19 Jan 2018 06:20
Uncontrolled Keywords: polarimetric, stars, evolution, magnetic field, rotation
Fields of Research : 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
Socio-Economic Objective: E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
Identification Number or DOI: 10.1093/mnras/stw3094
URI: http://eprints.usq.edu.au/id/eprint/33568

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