Stellar atmospheres

Part 1 — TABLE XV

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STELLAR ATMOSPHERES EDITOR’S FOREWORD

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TABLE I TABLE II TABLE III TABLE IV

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TABLE V TABLE VI TABLE VII TABLE VIII TABLE IX

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TABLE XI TABLE XII TABLE XIII TABLE XIV TABLE XV TABLE XVI

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TABLEXVIII TABLE XIX NOTES ON OBSERVATIONAL MATERIAL

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TABLE XX TABLE XXI TABLE XXII

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TABLE XXIII TABLE XXIV

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TABLE XXVII TABLE XXVIII TABLE XXIX

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TABLE XXX TABLE XXXI

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TABLE XXXII TABLE XXXIII TABLE XXXIV SUBJECT INDEX NAME INDEX

Series Wave-Lenght Int. Attribution Int. Wave-Lenght

3620.94 20 Y? 00 3621.110

3592.91 10 Y 0 3593.040

3552.69 3 - -

4128.32 30 00 4128.46

4039.83 5 Y 00 4040.013

4047.65 8 Y 4047.823

4102.38 20 Y 0 4102.541

4167.52 10 00 4167.737

4077.39 20 La, Y ? 4077.498

The multiplets at 4174, etc., and at 4674, etc., and the multiplets, do not appear in the solar spectrum. None of the above lines is strong enough to be seen in the spectra of the stars.

IONIZED YTTRIUM

Four of the multiplets attributed to ionized yttrium[334] are satisfactorily identified in the solar spectrum. The wave-lengths and identifications are contained in Table XVI, p. 83. The arrangement is as in Table XI.

Notes in this chapter

Note 1 · Ibid.

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