We determined the warp parameters of 192 warped galaxies which are selected from 340 edge-on galaxies using color images as well as r-band isophotal maps. We derive the local background density (∑ n) to examine the dependence of the warp amplitudes on the galaxy environment. We find a clear trend that strongly warped galaxies are likely to be found in high density regions where tidal interactions are supposed to be frequent. However, the correlation between αω and ∑ n is too weak for weakly warped galaxies (αω < 4◦) and the cumulative distributions of weakly warped galaxies are not significantly different from those of galaxies with no detectable warps. This suggests that tidal interactions do not play a decisive role in the formation of weak warps.

Abstract
1. INTRODUCTION
2. OBSERVATIONAL DATA
    2.1. Sample Selection
    2.2. Measurement ofWarp Parameters
3. BASIC PROPERTIES OF WARPED DISKS
    3.1. Warp Types
    3.2. Warp Angle
    3.3. Warp Radius
    3.4. Warp Asymmetry
    3.5. Morphological Types ofWarped Galaxies
4. ENVIRONMENTAL DEPENDENCE OF WARPAMPLITUDE
    4.1. Derivation of EnvironmentMeasures
    4.2. Frequency Distribution of the Local BackgroundDensity
    4.3. Correlation between EnvironmentMeasures andWarp Amplitude
    4.4. K-S Test
5. DISCUSSION AND CONCLUSIONS
REFERENCES

• Hong Bae Ann(Pusan National University) Corresponding author
• Hyun Jeong Bae(Pusan National University)