Mechanical equilibrium of hot, large-scale magnetic loops on T Tauri stars

A. Aarnio, J. Llama, M. Jardine, S. G. Gregory

Research output: Contribution to journalArticlepeer-review

7 Citations (Scopus)

Abstract

The most extended, closed magnetic loops inferred on T Tauri stars confine hot, X-ray-emitting plasma at distances from the stellar surface beyond the X-ray-bright corona and closed large-scale field, distances comparable to the corotation radius. Mechanical equilibrium models have shown that dense condensations, or 'slingshot prominences', can rise to great heights due to their density and temperatures cooler than their environs. On T Tauri stars, however, we detect plasma at temperatures hotter than the ambient coronal temperature. By previous model results, these loops should not reach the inferred heights of tens of stellar radii where they likely no longer have the support of the external field against magnetic tension. In this work, we consider the effects of a stellar wind and show that indeed hot loops that are negatively buoyant can attain a mechanical equilibrium at heights above the typical extent of the closed corona and the corotation radius.
Original languageEnglish
Pages (from-to)1797-1802
Number of pages6
JournalMonthly Notices of the Royal Astronomical Society
Volume421
Issue number2
DOIs
Publication statusPublished - Apr 2012

Keywords

  • stars: activity
  • stars: coronae
  • stars: flare
  • stars: magnetic field
  • stars: pre-main-sequence

Fingerprint Dive into the research topics of 'Mechanical equilibrium of hot, large-scale magnetic loops on T Tauri stars'. Together they form a unique fingerprint.

Cite this