Back to the article index

Table of Contents

ABSTRACT

1.INTRODUCTION

2.ANGULAR MOMENTUM EXCHANGE. ANALYTICAL RESULTS

3.ANGULAR MOMENTUM EXCHANGE. SIMULATION RESULTS

4.WHY IS THERE SUCH A WIDE VARIETY OF BAR STRENGTHS IN OBSERVED GALAXIES, AND WHY ARE SOME GALAXIES NON-BARRED ?

5.A BAR IN THE HALO

6.DO BARS FLATTEN OR STEEPEN CENTRAL HALO CUSPS?

REFERENCES