The intensity of quartet lines in the arc spectrum of copper

[1] The origin of the nebular lines and the structure of the planetary nebulae [J]. ASTROPHYSICAL JOURNAL, 1928, 67 (01) : 1 - 15

[2] DOBSON, PHOTOGRAPHIC PHOTOME, P77

[3] HARRISON, 1929, J OPT SOC AM, V18, P287

[4] HARRISON, 1929, J OPT SOC AM, V19, P109

[5] HYDE, 1917, PHYS REV, V10, P395

[6] KRONIG, 1925, Z PHYS, V33, P261

[7] NOTTINGHAM, 1929, J FRANK I, V207, P299

[8] NOTTINGHAM, 1928, B AM PHYS SOC, V3, P11

[9] RUSSELL, 1925, P NAT ACAD SCI, V11, P314

[1] The origin of the nebular lines and the structure of the planetary nebulae [J]. ASTROPHYSICAL JOURNAL, 1928, 67 (01) : 1 - 15

[2] DOBSON, PHOTOGRAPHIC PHOTOME, P77

[3] HARRISON, 1929, J OPT SOC AM, V18, P287

[4] HARRISON, 1929, J OPT SOC AM, V19, P109

[5] HYDE, 1917, PHYS REV, V10, P395

[6] KRONIG, 1925, Z PHYS, V33, P261

[7] NOTTINGHAM, 1929, J FRANK I, V207, P299

[8] NOTTINGHAM, 1928, B AM PHYS SOC, V3, P11

[9] RUSSELL, 1925, P NAT ACAD SCI, V11, P314