📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

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/10.5281/zenodo.61383

Publication URI: https://zenodo.org/record/61383

Type: Other