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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 1.1.The Need for Reliable Classification of Faint
Optical Galaxy Samples
- 1.2.UV Morphology of Nearby Galaxies as Benchmark for High
Redshift Classifications
- 1.3.Other Ways of Addressing the Morphological
K-correction
- 1.4.Goals of our HST Mid-UV Imaging Survey
- 2.STRATEGY, SAMPLE SELECTION AND
OBSERVATIONS
- 2.1.WFPC2 Mid-UV Survey Strategy
- 2.2.Sample Selection
- 2.3.Observations
- 2.4.Calibration and Processing of the
HST Observations
- 3.PRESENTATION OF THE WFPC2 MID-UV
IMAGES
- 4.DISCUSSION OF GENERAL TRENDS IN THE WFPC2
MID-UV IMAGES
- 4.1.Early-type Galaxies
- 4.2.Mid-type Spirals
- 4.3.Late-type Galaxies and Irregulars
- 4.4.Peculiars and Mergers
- 5.SUMMARY AND CONCLUSIONS
- REFERENCES