Imaging the cool stars in the interacting binaries AE Aqr, BV Cen and V426 Oph

Christopher Watson, D. Steeghs, V.S. Dhillon, T. Shahbaz

Research output: Contribution to journalArticlepeer-review

9 Citations (Scopus)

Abstract

It is well known that magnetic activity in late-type stars increases with increasing rotation rate. Using inversion techniques akin to medical imaging, the rotationally broadened profiles from such stars can be used to reconstruct `Doppler images' of the distribution of cool, dark starspots on their stellar surfaces. Interacting binaries, however, contain some of the most rapidly rotating late-type stars known and thus provide important tests of stellar dynamo models. Furthermore, magnetic activity is thought to play a key role in their evolution, behaviour and accretion dynamics. Despite this, we know comparatively little about the magnetic activity and its influence on such binaries. In this review we summarise the concepts behind indirect imaging of these systems, and present movies of the starspot distributions on the cool stars in some interacting binaries. We conclude with a look at the future opportunities that such studies may provide.
Original languageEnglish
Pages (from-to)813-816
Number of pages4
JournalAstronomische Nachrichten
Volume328
Issue number8
DOIs
Publication statusPublished - Jan 2007

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Fingerprint

Dive into the research topics of 'Imaging the cool stars in the interacting binaries AE Aqr, BV Cen and V426 Oph'. Together they form a unique fingerprint.

Cite this