*UBER DIE HAUFIGKEITSVERTEILUNG DER ABSOLUTEN HELLIGKEITEN DER F-STERNE

[1] BLAAUW A, 1948, B ASTRON I NETHERL, V10, P365

[2] BOK BJ, 1935, HARVARD CIRC, V400, P16

[3] BOSS B, 1938, ASTRONOMICAL J, V47, P125

[4] BOSS L, 1936, GENERAL CATALOGUE 33

[5] FLETSCHER A, 1932, MONTHLY NOTICES, V92, P780

[6] GYLLENBERG W, 1927, MEDD LUND OBS, V2

[7] RAYMOND H, 1915, AJ, V29, P25

[8] SMART WM, 1938, STELLAR DYNAMICS

[9] The distribution of absolute magnitudes among F and G stars brighter than the sixth apparent magnitude as determined from parallactic and peculiar velocities [J]. ASTROPHYSICAL JOURNAL, 1931, 74 (02) : 110 - 121

[10] VANDEKAMP P, 1936, ASTRON J, V45, P177

[1] BLAAUW A, 1948, B ASTRON I NETHERL, V10, P365

[2] BOK BJ, 1935, HARVARD CIRC, V400, P16

[3] BOSS B, 1938, ASTRONOMICAL J, V47, P125

[4] BOSS L, 1936, GENERAL CATALOGUE 33

[5] FLETSCHER A, 1932, MONTHLY NOTICES, V92, P780

[6] GYLLENBERG W, 1927, MEDD LUND OBS, V2

[7] RAYMOND H, 1915, AJ, V29, P25

[8] SMART WM, 1938, STELLAR DYNAMICS

[9] The distribution of absolute magnitudes among F and G stars brighter than the sixth apparent magnitude as determined from parallactic and peculiar velocities [J]. ASTROPHYSICAL JOURNAL, 1931, 74 (02) : 110 - 121

[10] VANDEKAMP P, 1936, ASTRON J, V45, P177