SUMMARY OF PROPOSAL 73001

FABIO FAVATA
FFAVATA@ASTRO.ESTEC.ESA.NL

EUROPEAN SPACE AGENCY
P.O. BOX 299
NOORDWIJK
NETH 2200 AG
Tel: +31-71-565 4665 Fax: +31-71-565 4690
Medium: CD ROM
Subject: STARS

THE FLARING BEHAVIOR OF DME STARS ACROSS A RANGE OF QUIESCENT X-RAY FLUXES


ABSTRACT

We propose observation of three well known, dMe single flare stars, spanning a factor of 100 in their quiescent X-ray flux. These observations will allow study of 1) the frequency of large and small flares, 2) the frequency-intensity relation, specially at the ``bright end'', and 3) the (possible) dependence of the flare frequency on quiescent X-ray luminosity. Recent observations of very large flares on dMe stars show large coronal mass ejections; a determination of the frequency of such events is critical for assessing their (possibly large) contribution to the chemical equilibrium of the interstellar medium. The detailed study of flaring events detected during the campaign will allow the sampling of extreme coronal conditions in a way not possible in other single stars.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
ANTONIO MAGGIOPALERMO ASTR. OBS.ITALY
GIUSEPPINA MICELAPALERMO ASTR. OBS.ITALY
SALVATORE SCIORTINOPALERMO ASTR. OBS.ITALY

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)EV LAC
B
341.7204 44.3403
80 ks
N
N
P
0.40000
1
2)PROXIMA CEN
B
217.4288-62.6797
80 ks
N
N
P
0.20000
1
3)AU MIC
C
311.2846-31.3359
80 ks
N
N
P
0.40000
1