Astron. Astrophys. 337, 757-771 (1998)
Prominence and plage activity in the recently discovered late-type rapid rotator, RE 1816+541
M.T. Eibe
Armagh Observatory, College Hill, Armagh BT61 9DG,
Northern Ireland
Received 6 May 1998 / Accepted 30 June 1998
Abstract
The rapidly-rotating, chromospherically active late-type star
RE 1816+541 has shown signs of intense magnetic activity in
various forms. Time-series of high resolution spectra have been
obtained during three nights and several important events were
detected. Observations contained several chromospheric lines, allowing
us investigate simultaneously the response of the chromosphere at
different heights.
A detailed analysis of the H line behaviour,
in particular, has revealed prominence clouds and plage-like regions
in this star. Rapid rotation favours detection and further
investigation of these features. Prominence clouds are seen to lie
below the co-rotation radius. A bright plage-like region was well
resolved on the first night. The feature disappeared temporarily
during meridian crossing, coinciding with the passage of a cloud.
Complete obscuration of the plage by the cloud proves that the
emission feature is located on or near the stellar surface, whereas
the cloud is at larger height and is seen in projection onto it. A
very large flare was also detected during the observations, having
strong effects in all the chromospheric lines selected for study.
Key words: stars:
activity
stars:
chromospheres
stars: individual:
RE 1816+541
starspots
Present address: LAEFF, Apdo 50727, E-28080 Madrid, Spain
Send offprint requests to: M.T. Eibe
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© European Southern Observatory (ESO) 1998
Online publication: August 27, 1998
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