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 language | English (US) |
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Pages (from-to) | L33-L36 |
Journal | Astrophysical Journal |
Volume | 420 |
Issue number | 1 PART 2 |
DOIs | |
State | Published - Jan 1 1994 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science