Viewing page 44 of 177

40

C-15533 ✓ mu phi 2509       350
#1    5 Serpentio, 5.74, GO

[[10 columned table]]
|Line|n|m+n|l+m+n|mean n|mean m+n|[n]|[m+n]|dm|dl|
|---|---|---|---|---|---|---|---|---|---|
|beta|140|180|350|140|180|66|45|21|18|
|gamma|170|220|350|170|220|50|26|24|20|
|delta|130|190|350|130|190|71|40|31|25|
|tau|30|140|350|30|140|148|66|82|83|
|kappa|20|120|350|20|120|162|76|90|56|
|xi|60|90|350|60|90|115|91|24|20|
|eta|20|30|350|20|50|-|125|-|   |

[[image - multi-line graph, C15533]]
C15533 
[[4 downslope lines]]
GO [[upward arrow on x-axis]]
KO [[upward arrow on y-axis]]

John G. Wolbach Library, Harvard-Smithsonian Center for Astrophysics • Provided by the NASA Astrophysics Daya System

Transcription Notes:
Greek letters in the first table column.

Please note that the language and terminology used in this collection reflects the context and culture of the time of its creation, and may include culturally sensitive information. As an historical document, its contents may be at odds with contemporary views and terminology. The information within this collection does not reflect the views of the Smithsonian Institution, but is available in its original form to facilitate research. For questions or comments regarding sensitive content, access, and use related to this collection, please contact transcribe@si.edu.