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1971, Astrophys. J. Letters 165, L49. Haggerty, M. J. and Wertz, J. : 1972, Monthly Notices Roy. Astron. Soc. 155, 495. : 1967, Compt. Rend. A cad. Sci. Paris 263B, 1186. : 1969, Astrophys. Letters 3, 19. : 1971, Mem. Roy. Astron. Soc. 75, Parts 4-6, 85, 105, 121. : 1969, Astrophys. Letters 3, 153, and Thesis, Univ. of Paris. , London. Hodge, P. : 1961, Astron. J. 66, 249, 384. Hodge, P. : 1963, Astron. J. 68, 470. Hodge, P. : 1964, Astron. J. 69, 438. Hodge, P. : 1965, Astrophys. J. 142, 1390.

8 log A {kpc} Correlation between absolute magnitude MB and length scale a-I = A (kpc). 65 mag (arc sec)-2. tion of objects for detailed photometry (there is very little photometry of low-surfacebrightness objects)? 30 mag or, again, is it a result of selection effects in a small sample (8 objects out of 36 were rejected in the analysis)? 5 mag(arc sec)-2 (de Vaucouleurs, 1969); the elongated shape of the isophotes (Arp and Bertola, 1969, 1971) suggests that the coronas are flattened; (2) comparison of several late-type spirals and irregulars with pure exponential distributions (de Vaucouleurs and Freeman, 1972, Fig.

J. 71, 231. : 1936, Astrophys. J. 84, 158. : 1973, Astron. Astrophys. 22, 91. Humason, M. , Mayall, N. , and Sandage, A. : 1956, Astral!. J. 61, 97. Johnson, H. : 1966, Astrophys. J. 143, 187. Johnson, H. : 1961, Astrophys. J. 133, 314. Karachentsev, I. : 1967, Commun. Byurakal! Obs. 39, 96. Karachentseva, V. : 1967, Astrofizika 3, 535. Karachentseva, V. : 1972, in Problems of Cosmical Physics, Kiev Univ. Publ. 7, p. 150. : 1971, Astrophys. J. Letters 165, L49. Kerr, F. : 1973, Report to Commission 40, IAU meeting, Sydney.

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