CONTINUOUS EMISSION FROM PLANETARY NEBULAE

[1] BETHE, 1933, HDB PHYS, V24, P442

[2] Metastability of hydrogen and helium levels [J]. ASTROPHYSICAL JOURNAL, 1940, 91 (02) : 215 - 238

[3] NEGATIVE HYDROGEN IONS IN PLANETARY NEBULAE [J]. ASTROPHYSICAL JOURNAL, 1951, 114 (01) : 106 - 109

[4] CONTINUOUS EMISSION IN THE ORION NEBULA [J]. ASTROPHYSICAL JOURNAL, 1946, 104 (03) : 414 - &

[5] The doppler effect in resonance lines [J]. PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1940, 26 : 50 - 54

[6] KIPPER, 1950, AJ USSR, V27, P321

[7] FINE STRUCTURE OF THE HYDROGEN ATOM BY A MICROWAVE METHOD [J]. PHYSICAL REVIEW, 1947, 72 (03): : 241 - 243

[8] LUDERS G, 1950, Z NATURFORSCH A, V5, P608

[9] MEYER, 1931, ANN PHYS, V9, P273

[10] Minkowski R, 1942, ASTROPHYS J, V96, P199, DOI 10.1086/144447

[1] BETHE, 1933, HDB PHYS, V24, P442

[2] Metastability of hydrogen and helium levels [J]. ASTROPHYSICAL JOURNAL, 1940, 91 (02) : 215 - 238

[3] NEGATIVE HYDROGEN IONS IN PLANETARY NEBULAE [J]. ASTROPHYSICAL JOURNAL, 1951, 114 (01) : 106 - 109

[4] CONTINUOUS EMISSION IN THE ORION NEBULA [J]. ASTROPHYSICAL JOURNAL, 1946, 104 (03) : 414 - &

[5] The doppler effect in resonance lines [J]. PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1940, 26 : 50 - 54

[6] KIPPER, 1950, AJ USSR, V27, P321

[7] FINE STRUCTURE OF THE HYDROGEN ATOM BY A MICROWAVE METHOD [J]. PHYSICAL REVIEW, 1947, 72 (03): : 241 - 243

[8] LUDERS G, 1950, Z NATURFORSCH A, V5, P608

[9] MEYER, 1931, ANN PHYS, V9, P273

[10] Minkowski R, 1942, ASTROPHYS J, V96, P199, DOI 10.1086/144447