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The multipolar magnetic fields of accreting pre-main-sequence stars: B at the inner disk, B along the accretion flow, and B at the accretion shock (2016)

First Author: Gregory S

Attributed to: Magnetic fields: the key to understanding the physics of stellar evolution and exoplanetary systems funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1609.00273

Publication URI: https://arxiv.org/abs/1609.00273

Type: Preprint