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  • NAM2017
    • Timetable
    • Delegates
    • Registration
  • Science
    • Parallel sessions
    • Plenary talks
    • Posters
    • Publishing workshop
    • Media workshop
    • Community forum
    • Special lunches
    • Hack day
  • Social
    • Welcome reception
    • Conference dinner
    • Football + BBQ evening
  • Outreach
    • Public talk
    • Outreach day
    • Media
  • Hull
    • Travel
    • Accommodation
    • Going out
    • Childcare
  • Contacts

Tuesday

Abstract

id
The magnetic and coronal evolution of pre-main sequence stars
Generation and evolution of Solar and Stellar Magnetic Fields, and Implications for the Solar-Stellar Connection
Date Submitted
2017-04-14 12:23:51
Scott G. Gregory
University of St Andrews
Forming low-mass stars appear to be born with simple, dominantly axisymmetric, large-scale magnetic fields. Their magnetospheres transition to complex, multipolar, and dominantly non-axisymmetric, as they evolve across the H-R diagram towards the main sequence. I will discuss the evolution of stellar magnetism during the pre-main sequence phase and the implications this has for coronal X-ray emission. I will highlight some recent observations that may suggest that magnetospheric accretion during the star-disk interaction phase influences the magnetic topology of young stars.

Schedule

id
date time
09:00 - 10:30
09:00
Abstract
The magnetic and coronal evolution of pre-main sequence stars
Tuesday
Wilberforce LT-1

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