Photoelectric drift scans of nearby galaxies, M106, M31 and M33 have been made at diurnal rate with the 61cm Cassegrain Reflector at Sobacksan Observing Station. Luminosity profiles of M106 and M31 show the asymmetries between east and west sides of the galaxies and the near side of each galaxy exhibits a larger B-V color than the far side. B-V color distribution in the central part of MI06 shows somewhat unusual feature of a blue center with red surrounding regions, and this is an opposite trend to the ordinary color distribution of most of external galaxies. B-V color of M31 is nearly constant in the central part of the galaxy while U-B color decreases as the distance from the center increases.

ABSTRACT
Ⅰ. INTRODUCTION
Ⅱ. OBSERVATIONS
Ⅲ. DATA REDUCTION
Ⅳ. RESLTS AND DISCUSSION
Ⅴ. CONCLUDING REMARKS
REFERENCES

• H. B. ANN(Department of Astronomy, College of Natural Sciences, Seoul National University)
• K. L. YU(Department of Astronomy, College of Natural Sciences, Seoul National University)