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Table of contents

Barred Magellanic Spirals in Ursa Major and Canes Venatici: Global Properties

Motivation

Barred Magellanic Spirals (SBms)

H I emission

Observing H I with the VLA

NGC 3264

NGC 4288

NGC 4861

Conclusions

Further Work

Acknowledgments

This Experience

Some Optical Images

Author: Kwayera Davis

E-mail: cosmickiwidude@yahoo.com

Homepage: http://wisp.physics.wisc.edu/~reu2003/davis/index.html