Viewing page 107 of 112

This transcription has been completed. Contact us with corrections.

[[preprinted]] 210 [[/preprinted]]

May 20, '97

gamma Tuc. [[strikethough]] 5988 1 [[superscript]] 4 [[/superscript]][[/strikethrough]] 5392 1 [[superscript]] 4 [[/superscript]]
K slightly stronger than H.
K = 3 H gamma
H delta is narrower than H gamma

gamma Tuc. 5988 1 [[superscript]] 4 [[/superscript]]
Solar lines not so clearly seen as in 5392
This ^[[star]] seems a little nearer alpha Canis Maj. than theta Scorpii does. The lines, F, G & h are a little weaker and k is slightly stronger and the lines that form the G band seem to be a little crowded together.

gamma Tuc. 7830 2 [[superscript]] 3 [[/superscript]]

[[end page]]
[[start page]]

[[preprinted]] 211 [[/preprinted]]

[[underline]] May 21, '97 [[/underline]]

7308 1 [[superscript]] 3 [[/superscript]] A.G.C 608 The only plate. Poor spectrum
Probably under alpha Bootis. Hyd. lines rather strong.

7308 1 [[superscript]] 3 [[/superscript]] A.G.C. 544 (also on plate) Probably under alpha Bootis. Spectrum poor, on edge of plate.

7834 2 [[superscript]] 4 [[/superscript]] pi Sag.
K = H = 3F, G & h
lines are sharp. The slightest indication of the g band is seen.

omicron Sag. also on plate at top and spectrum is faint.

alpha Hydri 8017 2 [[superscript]] 4 [[/superscript]]
K = 1.1 H.
Hyd. lines especially towards violet are hazy and solar lines look almost double. Is it focus? There seems to be a sort of banding extending over most of the spectrum. A similar effect was observed in alpha Circini 6400.