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A far-ultraviolet flare on a pleiades G dwarf

  • T. R. Ayres
  • , J. R. Stauffer
  • , Theodore Simon
  • , R. A. Stern
  • , S. K. Antiochos
  • , G. S. Basri
  • , J. A. Bookbinder
  • , A. Brown
  • , G. A. Doschek
  • , J. L. Linsky
  • , L. W. Ramsey
  • , F. M. Walter
  • University of Colorado Boulder
  • Harvard-Smithsonian Ctr. Astrophys.
  • University of Hawai'i at Mānoa
  • Lockheed Martin
  • Naval Research Laboratory
  • University of California at Berkeley
  • Natl. Inst. of Std. and Technology
  • Pennsylvania State University

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

The HST/FOS recorded a remarkable transient brightening in the C IV λλ1548,50 emissions of the rapidly rotating Pleiades G dwarf H II 314. On the one hand the "flare" might be a rare event luckily observed; on the other hand it might be a bellwether of the coronal heating in very young solar-mass stars. If the latter, flaring provides a natural spin-down mechanism through associated sporadic magnetospheric mass loss.

Original languageEnglish
Pages (from-to)L33-L36
JournalAstrophysical Journal
Volume420
Issue number1 PART 2
DOIs
StatePublished - Jan 1 1994

Keywords

  • Stars: coronae
  • Stars: flare
  • Stars: mass loss
  • Stars: rotation
  • Ultraviolet: stars

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