By M. Rodonò (auth.), Patrick B. Byrne, Marcello Rodonò (eds.)
IAU Colloquium No. seventy one had its instant origins in a small collecting of individuals . within the optical and UV examine of flare stars which happened throughout the 1979 Montreal common meeting. We famous basic swap was once occurring within the examine of those gadgets. Space-borne tools (especially lUE and Einstein) and a brand new genera tion of ground-based gear have been having a profound influence at the diversity of investigations it used to be attainable to make. To extract greatest reap the benefits of those new percentages it might be worthwhile as by no means prior to to have solid conversation with colleagues in different disciplines, for instance,. with atomic and sunlight physicists. equally, reviews of phenomena linked to the outer atmospheres of the late-type stars may perhaps now wish to offer major insights into definite features of sun job. So, in view of the wide variety of backgrounds of these engaging, the assembly had an strangely excessive share of invited stories whereas many of the contributed papers have been provided as posters. it truly is enjoyable that during the quick time because the assembly a great deal of correspondence has been got from contributors remarking at the good fortune of this structure. as soon as the choice were taken in precept to carry the assembly, a truly significant quantity of labor fell at the organizing committees, viz. the clinical and native Organizing Committees. The medical Organizing Committee used to be chaired through D.J. Mullan and consisted of A.D.
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Extra info for Activity in Red-Dwarf Stars: Proceedings of the 71st Colloquium of the International Astronomical Union Held in Catania, Italy, August 10–13, 1982
249, LS. , and Vaiana, G. : 1982, /Jp. J, (in press). Roxburgh, 1: 1983, in Stenflo (1983). Schmitt, J. H. M. : 1982, /Jp. , in press. : 1983, in Stenflo (1983). Jp. , 171, 565. : 1983, in Stenflo (1983). Spruit, H. : 1983, in Stenflo (1983). Spiegel, E. , and Weiss, N. re, 287, 616. Spiegel, E. , and Weiss, N. : 1981, Columbia Univ. Preprint No. AlO. II and Coroaal Effects, editor (Dordrech t: Reidel), in press. Tarbell, T. : 1983, in Stenflo (1983). : 1982, IJp. , in press. Vaiana, G. : 1981, but.
386 valid for 8<~<19. 27. -6,---------------------------, BC -5 -4 0 3 4 5 6 (V-K) Fig. 4. B 9 Bolametrie eorreetion versus the (V-K) eolour index. PARAMETERS OF ACTIVE DWARF STARS 21 The relations between BC and colour indices also show no deviation from linearity (Figure 4). Table 2 gives the results of the least square analyses. A comparison with the (BC, colour)-relations of Johnson (1965) reveals good correspondance for BC~-2. For BC<-2 Johnson's (1965) values of BC for a given value of a colour index are consistently smaller than our values.
1980, PIJSP, 92, 235. Walter, F. Jp. , MS, 677. Walter, F. : 1981, /Jp. , MS, 671. Willson, R. , Hudaon, H. , and Chapman, G. : 1981, Science, 211, 700. Wilson, 0. Jp. , 144, 695. : 1983, in Stenflo (1983). MAGNETIC FIELDS AND ACTIVITY OF THE SUN AND STARS 13 DISGUSSION Mullan: Can I ask whether there 1s a connection between flares and coronal heating or do you thing that those topics should be discussed separately? Rosner: I don't think that they are intimately related. Clearly there is a relation.