We studied a cluster family in the northern part of the Carina Nebula (NGC 3372) a group of clusters near NGC 3324 (Tr 15, NGC 3293, Loden 165, Loden 153 and IC 2581). We used data from UCAC4 to determine the cluster's membership and the near infrared CMDs of each cluster. We analyzed the spatial density and elongation as a function of radius for each cluster and found a possible interaction between NGC 3293 and Loden153. However, the shape distortion of NGC 3324 cannot be evaluated because of the inhomogenity in the coverage of UCAC4 in the east part of NGC 3324.

ABSTRACT
1. INTRODUCTION
2. DATA
3. METHOD
4. RESULTS AND DISCUSSION
REFERENCES

• Ramadhani Putri Ayu(Astronomy Program, Institut Teknologi Bandung)
• Rhorom Priyatikanto(Astronomy Program, Institut Teknologi Bandung/National Institute of Aeronautics and Space)
• M. Ikbal Arifyanto(Astronomy Program, Institut Teknologi Bandung)
• Riska Wahyu Romadhonia(Astronomy Program, Institut Teknologi Bandung)
• Miftahul Hilmi(Astronomy Program, Institut Teknologi Bandung)
• Itsna Khoirul Fitriana(Astronomy Program, Institut Teknologi Bandung)
• Hesti R. T. Wulandari(Astronomy Program, Institut Teknologi Bandung)