... an extraordinary endeavour, in light of what we have learnt about Solar System planets, only a handful of key ingredients are ... significant stellar variability (due to star spots and flares) that render the search for transiting planets challenging ...
... to account for the double-peaked radio flares from Cir X-1, observed at multi ... X-ray properties seem to indicate some few solar masses for the primary star Stewart ... At 1.4 and 2.3 GHz the flare is broad and does not seem to have double-peaked ...
... to account for the doublepeaked radio flares from Cir X1, observed at multi ... Xray properties seem to indicate some few solar masses for the primary star Stewart ... b) At 1.4 and 2.3 GHz the flare is broad and does not seem to have doublepeaked ...