... COSPAR Session E0.1:"Connections and reconnections in solar and stellar coronae". Houston, TX, USA, 10-19 October 2002. ... In: "Stellar Coronae in the Chandra and XMM-Newton era". ASP Conference Proceedings, Vol. ...
... The 35th ESLAB Symposium "Stellar Coronae in the Chandra and XMM-Newton era" . ... In: "Stellar Coronae in the Chandra and XMM-Newton era" . ... COSPAR Session E0.1:"Connections and reconnections in solar and stellar coronae". ...
... M.M.Katsova, V.Tsikoudi, M.A.Livshits "New effects in the IRAS data and their consequences for coronae of active late-type stars" in: Physics of Solar and Stellar Coronae: G.S.Vaiana Memorial Symp. ...
... properties are closely tied to the corona; furthermore, they vary in a well-defined ... the common physical connection between the corona, the accretion disk, and the jet ...
... the energy flux per unit surface area of the corona Qcor , the radiation energy density ( ), and electron temperature Te is ... d 2 3Qtot =- , (2) d 2 c0 where Qtot = Qcor + Qdisk is the sum of the corona (TL) and intercepted disk fluxes, respectively ...
... in the 2550 keV band with INTEGRAL, Cherepashchuk et al. (2007) and Krivosheyev et al. (2009) propose that a hot extended corona around the accretion disk is responsible for the hard X-ray emission via thermal Comptonization with a temperature of 20 keV ...