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[[preprinted]] 162 [[/preprinted]] May 3, '97 beta Grucis 7914 2 [[superscript]] 3 [[/superscript]] " " [[dittos for beta Grucis]] 7659 2 [[superscript]] 4 [[/superscript]] " " [[dittos for beta Grucis] 4296 1 [[superscript]] ? [[/superscript]] " " [[dittos for beta Grucis] 7899 2 [[superscript]] 3 [[/superscript]] " " [[dittos for beta Grucis] 7829 2 [[superscript]] 4 [[/superscript]] In 7829, the two bands I & bet. I & II are the only conspicuous marking at the red end. They seem about equally strong. There is only a slight change in light at 4307. The G band consists of two wide lines, the narrower one seen in gamma Crucis having almost disappeared. beta Grucis probably forms ^[[one]] the group following alpha orionis. On 5650, there is a tendency to show a break near the lambda 4762, about .18 mm nearer the red end of spectrum. Is this characteristic of stars beyond alpha Orionis? [[end page]] [[start page]] [[preprinted]] 163 [[/preprinted]] May 3, 97 sigma Librae 418 [[strikethrough]] 7 [[/strikethrough]] 6 1 [[superscript]] ? [[/superscript]] poor. Under alpha Orionis? sigma Librae 418 [[strikethrough]] 6 [[/strikethrough]] 7 4227.0 2 as strong as in alpha Orionis. No lines are sharp in absorption bands. I, I-II, & III of nearly equal brightness. Is this star beyond alpha Orionis? gamma Hydr[[strikethrough]]ae[[/strikethrough]]^[[I]] 4336 too poor. sigma Librae 5614 1 [[superscript]] 3 [[/superscript]] best plate. Spectrum seen to lambda 4954 The new band I to II is getting brighter, is clearly intermediate between I & II. II has faded H lines. H gamma slightly [[strikethrough]] bright [[/strikethrough]] stronger than 4326.0 Lines are certainly seen in the absorption bands. I think this star should go in same class as alpha Orionis. 1st type star is faint on this plate.