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7 [[2 Columned Table]] --- | --- | B7859 9.18 | c 4 s.v 9.58 9.60 9.62 = 9.60 [[underlined]].02[[/underlined]] .00 .02 🗸 9.60 | s.v o d 9.60 9.62 | s.v 4 e 10.02 | B4826 9.18 | C 5s.v 9.68 9.60 9.62 = 963 .05 [[underlined]].03[[/underlined]] [[underlined]].01[[/underlined]] 🗸 9.60 | s.v o d 9.60 9.62 | s.v 4 e 10.02 | B7570 9.60 | d 1 s.v [[strikethrough]] 9.61 [[/strikethrough]] 9.70 9.72 = 9.71 [[underlined]].01[[/underlined]] .01 🗸 9.72 | s.v 3 e 10.02 | B3358 9.60 | d 3 s.v 9.90 9.82 = 9.86 .04 [[underlined]].04[[/underlined]] 🗸 9.82 | s.v 2 e 10.02 | B4871 Sp. 🗸 | too poor. | B4839 Sp. 🗸 | too poor | B4874 Sp. 🗸 | too poor. | B [[strikethrough]]3935[[/strikethrough]] 3395 Sp. 🗸 | too poor. | B5446 Sp 🗸 | too poor John G. Wolbach, Harvard-Smithsonian Center for Astrophysics • Provided by the NASA Astrophysics Data System
Transcription Notes:
Need heading formatting; need in several places, too.