ARE NEARBY SMALL-GROUPS OF GALAXIES EXPANDING WITH UNIVERSE

[1] CHINCARINI C, 1975, M NOT R AST, V70, P441

[2] STUDY OF 3 GROUPS OF GALAXIES - PLAUSIBLE EXPLANATION OF VIRIAL MASS DISCREPANCY [J]. ASTROPHYSICAL JOURNAL, 1973, 186 (03) : 777 - 785

[3] JACKSON JC, 1972, M NOT R AST, V156

[4] EMPIRICAL PROPERTIES OF MASS DISCREPANCY IN GROUPS AND CLUSTERS OF GALAXIES [J]. ASTROPHYSICAL JOURNAL, 1970, 162 (02) : 411 - &

[5] TURNER EL, 1974, ASTROPHYS J, V94, P587

[6] VAUCOULEURS AD, 1967, ASTRON J, V72, P730

[7] VAUCOULEURS AD, 1964, REFERENCE CATALOGUE

[8] VAUCOULEURS GD, 1975, STARS STELLAR SYSTEM, V9

[1] CHINCARINI C, 1975, M NOT R AST, V70, P441

[2] STUDY OF 3 GROUPS OF GALAXIES - PLAUSIBLE EXPLANATION OF VIRIAL MASS DISCREPANCY [J]. ASTROPHYSICAL JOURNAL, 1973, 186 (03) : 777 - 785

[3] JACKSON JC, 1972, M NOT R AST, V156

[4] EMPIRICAL PROPERTIES OF MASS DISCREPANCY IN GROUPS AND CLUSTERS OF GALAXIES [J]. ASTROPHYSICAL JOURNAL, 1970, 162 (02) : 411 - &

[5] TURNER EL, 1974, ASTROPHYS J, V94, P587

[6] VAUCOULEURS AD, 1967, ASTRON J, V72, P730

[7] VAUCOULEURS AD, 1964, REFERENCE CATALOGUE

[8] VAUCOULEURS GD, 1975, STARS STELLAR SYSTEM, V9