Viewing page 14 of 98

This transcription has been completed. Contact us with corrections.

[[preprinted]] 26 [[/preprinted]]

Dec. 9, 1897

X 6294 1 [[superscript]] 5 [[/superscript]] beta Muscae

B3A. lines little broad as if focus were out.

X 6153 1 [[superscript]] 5 [[/superscript nu Puppis
B8A.

X 4734 1 [[superscript]] 3i [[/superscript]] mu Crucis

Double star
[[margin]] A.G.C. 17542 [[/margin]]
Fainter component has
H beta bright
H gamma very wide
H delta  " "[[ditto for very wide]]
H epsilon faint
H zeta strong appears to be superposed on a faint line in sp. of the brighter component. This line is seen in alpha Muscae X 6486.
H eta is lost [[strikethrough]] by [[/strikethrough]] probably being superposed on 3819 - which is strong in the brighter star.

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

[[preprinted]] 27 [[/preprinted]]

Dec. 9, 1897.

X 4734 1 [[superscript]] 3i [[/superscript]] mu Crucis
[[margin]] A.G.C. 17541 [[/margin]]
Brighter component (mag. 4.4)
B3A
No lines are seen belonging to the fainter component except the hydrogen.

[[margin]] A.G.C. 17572 [[/margin]]
Other star on plate has the new series of hydrogen lines like zeta Puppis. This star is like [[strikethrough]] 30 [[/strikethrough]] tau Can. Maj. X 6265
The bright band