Part I the Nature of the Span Classsearchtermclassspan N Spectrum Part
Part I the Nature of the Span Classsearchtermclassspan N Spectrum Part
C D Shane
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J n-7 ft, / ^ . 2. 2. n. / 2. >a *7 yO 10 W ^"7. 7 % 1*3 -777 i*3 7 tf zy. F Jl '&* ft G //? /e> ;7 (>t. I>l i 10, 2- 23, 7 tf J n 2- US 33. I i'G W ft _j 1 Hit Co 01. 13 3V, i 2. \ fj 3)3 IcL *. 1 l( \^ \Kr 1 34- 1 I rf'*X I m? / rai'. Ff i 2 i J X. i. I. Q ' tess, t% \ U?f m IM^O i Kr & /' up;. ^7. 7^ . /', JJ. V 4A JV . 72- ^ j. 1 4- ?^7 ' "V^L f 1 fx. . 6^. 77 f7. // U3 I P 6J"J a i 7V>7 4 ? /? ? * V H j Part II. Variations in t -tra of Class H Variables Introduction It won i natural . :iat... s star whose light varies by a factor five or ten should show some changes in its spectrum during the variation, unless t 'is is effected thi o-. -.^'h the occulta^ion of Uio star by opaque matter* r Jhc lo od variables of Class Ud have been studied with particular reference Lr spectral changes by a number of observers, notebly 3 idgreaves^, U bobbins * T-f A Plaskett 13 '^rrill . ^. L though. Our knowledge of those stars is still far from factor, ; . 1 character of the v&riat io. Ua in thear Bj.
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