Sco 4492 3.1 -3.9 Ind 5281 3.2 2.5 Pav 4778 var. 0.0 Aqr 5963 3.8 0.5 Tuc 55 4.3 10.9 Gru 5965 4.1 4.9 For 723 4.0 8.3 Cru 3218 3.6 5.1 Lep 1420 3.8 9.7,7.1 Mus 3377 3.6 5.7 CMa 1839 2.0 -4.5 TrA 4250 1.9 -0.6 Hyi 74 2.9 9.7 Ara 4406 2.8 0.6 Aur 1246 0.2 3.4 Tuc 5747 2.9 2.6 Lep 1323 3.0 2.9 Tau 1077 1.1 2.6 Pup 2065 3.5 -2.3 Pup 1896 2.7 -2.8 Leo 2618 3.1 1.5 Pup 1972 3.3 4.7 Car 2628 var. 1.1 Car 2739 3.4 1.7 Cap 5507 3.9 (1.1) Apo 3746 3.8 1.4 Ret 994 3.4 2.6 Ara 4265 3.7 2.5 Vel 2875 2.8 2.3 Sco 4292 3.8 5.9 Hya 3042 3.7 5.3 Ara 4304 3.1 1.5 Crv 3280 2.8 1.7 And 259 2.4 -0.8 Hya 3449 3.3 2.9 Hyi 899 3.2 -1.3 CrA 4871 4.2 2.0 Ori 1468 0.9 -0.0 Pav 5138 3.6 9.7 Sco 4193 1.2 -2.5 Phe 78 2.4 5.6 Eri 759 4.0 3.2 Cas 135 2.5 1.4 Cru 3263 1.6 3.8 Phe 245 3.4 1.6 Lib 3837 3.4 3.3 Phe 336 4.0 5.4 Her 4373 3.5 0.9 Ret 875 3.8 6.2 Sgr 4617 3.2 4.9 Lep 1456 39 8.1 Gru 5854 2.2 2.8 Col 1459 3.2 6.2 [Pg 207] IV. INTENSITY CHANGES OF LINES WITH UNKNOWN SERIES RELATIONS THE following tabulation shows the intensity changes of lines of unknown series relations that occur in the hotter stars. The arrangement follows that of Table XIX. Notes on the maxima and blends are appended. TABLE XXXIII Atom Line Pup Note C++ 4649 0.0 2.0 9.0 6.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 .. 1 N+ 3996.9 0.0 0.0 0.0 0.0 5.0 6.0 7.0 .. 9.0 .. .. 5.0 0.0 1 N++ 4515.0 .. 9.0 4.0 4.0 1.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 2 4097.5 .. 15.0 8.0 5.0 .. 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 3 O+ 4943.4 0.0 0.0 0.0 0.0 4.0 4.0 3.0 0.0 0.0 0.0 0.0 0.0 0.0 1 4941.2 4705.3 0.0 0.0 0.0 2.0 4.0 4.0 3.0 0.0 0.0 0.0 0.0 0.0 0.0 2 4699.2 4676.2 0.0 0.0 0.0 2.0 5.0 .. 7.0 0.0 0.0 0.0 0.0 0.0 0.0 3 4661.6 0.0 0.0 0.0 2.0 5.0 .. 7.0 0.0 0.0 0.0 0.0 0.0 0.0 4 4649.1 0.0 0.0 0.0 6.0 9.0 12.0 9.0 .. 4.0 0.0 0.0 0.0 0.0 5 4641.8 0.0 0.0 0.0 0.0 3.0 10.0 7.0 .. 0.0 0.0 0.0 0.0 0.0 6 4596.2 0.0 0.0 0.0 1.0 5.0 .. 6.0 .. 3.0 0.0 0.0 0.0 0.0 7 4591.0 0.0 0.0 0.0 1.0 5.0 .. 6.0 .. 3.0 0.0 0.0 0.0 0.0 8 4417.0 0.0 0.0 0.0 5.0 6.0 11.0 3.0 .. 2.0 0.0 0.0 0.0 0.0 9 4415.9 0.0 0.0 0.0 3.0 .. 2.0 0.0 0.0 0.0 0.0 10 4366.9 0.0 4.0 4.0 4.0 .. 6.0 6.0 .. 1.0 0.0 0.0 0.0 0.0 11 4075.9 0.0 3.0 0.0 2.0 6.0 8.0 6.0 0.0 0.0 0.0 0.0 0.0 0.0 12 4072.2 0.0 0.0 0.0 2.0 7.0 9.0 6.0 0.0 0.0 0.0 0.0 0.0 0.0 13 4069.9 0.0 0.0 0.0 4.0 6.0 8.0 6.0 0.0 0.0 0.0 0.0 0.0 0.0 14 S+ 4815 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 x 0.0 0.0 0.0 1 4174.5 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 3.0 0.0 0.0 0.0 2 4162.9 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 3.0 0.0 0.0 0.0 3 S++ 4295 0.0 0.0 0.0 0.0 0.0 1.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 4 4285.0 0.0 0.0 0.0 0.0 0.0 6.0 4.0 0.0 0.0 0.0 0.0 0.0 0.0 5 4253.8 0.0 0.0 0.0 0.0 6.2 6.8 6.0 0.0 0.0 0.0 0.0 0.0 0.0 6 NOTES TO TABLE XXXIII Atom Note Maximum Remarks C++ 1 Line blended, in stars cooler than , with V+ 4649.1. Attributed by Fowler and Milne, and by Hartree, to C+++ N+ 1 Unblended N++ 2 3