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[[preprinted]] 14 [[/preprinted]] Jan. 8, 1908 C17181 (cont.) [[symbol-check mark]] (2) H Beta strength bright. H Gamma faint lines [[margin]]+ 62 degrees 2007 H.P. 3879 [[/margin]] Spectrum resembles that of long period variables. Not in Second Cat. Var. stars Identify on I 11688 [[symbol-check mark]] Sp. marked by W.P.F. on I 13536, Ma, object 3989, no bright lines Plates examined [[margin]] Aug. 21 ? [[/margin]] AI 2652 "[[ditto for Aug]] 7, 1907 6028 Jun 4, "[[ditto for 1907]] 6278 "[[ditto for Jun]] 8, "[[ditto for 1907]] 6290 "[[ditto for Jun]] 9, "[[ditto for 1907]] 6293 "[[ditto for Jun]] 11, "[[ditto for 1907]] 6298 "[[ditto for Jun]] 20, "[[ditto for 1907]] 6328 "[[ditto for Jun]] 27, "[[ditto for 1907]] 6336 Taken the same night as C17181 - [[margin]][Variable - confirmed by by W..P.F on I 29286, 13461, 16274, 16446, 13536,24137 Bright on I 29286, [[strikethrough]] 13461, 16274, 16446 [[/strikethrough]] Ft. on 13461, also conf. by E.F.L]] AC 7807, 8592, 8659, 8965, 9008, + 9073 The above plates show no change in this object. It is certainly no brighter on AI 6336 taken the night on which the C plate shows H beta bright than on other AI plates. Therefore it seems that the brightening of the hydrogen lines did not cause variation in light. [[End Page]] [[Start Page]] [[preprinted]] 15 [[/preprinted]] Jan. 8, 1908 [[symbol-check mark]] C17182 H.P. 264 1 [[underlined]] st [[/underlined]] type. Lines burned out. [[symbol-check mark]] C17183 H.P. 596 comp. would be F5G except that K is almost missing. [[symbol-check mark]] (2) H.P. 583 Ma [[symbol-check mark]] (3) +62^[[0]] 612 A3F [[symbol-check mark]] C17186 H.P. 4146 B9H? Very dense C17188 delta Cephei [[symbol-check mark]] C17190 H.P. 3172, 3173 H.P. 3172 A2F H.P. 3173 A3F Partly superposed [[End Page]]
Transcription Notes:
ditto words need doing as per instructions
changed to actual words for dittos see other examples
