III. Researches in spectrum analysis in connection with the spectrum of the sun
1878 ◽
Vol 27
(185-189)
◽
pp. 49-50
The author refers to the work already done in the new map of the Solar Spectrum as enabling the chemical constitution of the Sun’s atmosphere to be studied under more favourable conditions. He shows that, the work already done enables him to confirm the presence of Sr, Pb, Cd, K, Ce and U, and also that it indicates the probability of the presence of Va, Pd, Mo, In, Li, Rb, Cs, Bi, Sn, La, Gl, Yt or Er.
1881 ◽
Vol 172
◽
pp. 561-576
◽
1878 ◽
Vol 27
(185-189)
◽
pp. 279-284
1877 ◽
Vol 25
(171-178)
◽
pp. 546-546
1878 ◽
Vol 27
(185-189)
◽
pp. 409-409
◽
2014 ◽
Vol 10
(S305)
◽
pp. 381-386
1886 ◽
Vol 32
(3)
◽
pp. 519-543
◽