The nearby field galaxy survey: a spectrophotometric study of 196 galaxies in the local field

Rolf Arthur Jansen

The nearby field galaxy survey: a spectrophotometric study of 196 galaxies in the local field

Rolf Arthur Jansen

Research output: Thesis › Thesis fully internal (DIV)

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Abstract

The purpose of the present study is to accurately describe the distribution in the local galaxy population of (1) the magnitudes and colors, (2) emission and absorption line strengths, (3) star formation rate and star formation history, (4) morphology, and (5) structural parameters. zie: Chapter 1, introduction

Original language	English
Qualification	Doctor of Philosophy
Publisher	s.n.
Print ISBNs	9036713110
Publication status	Published - 2000

Keywords

Proefschriften (vorm)
Sterrenstelsels
39.41

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acknowledgements.pdfFinal publisher's version, 19.6 KB
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publications.pdfFinal publisher's version, 21 KB
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stelling.pdfFinal publisher's version, 10.4 KB
thesis.pdfFinal publisher's version, 19.4 MB

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Cite this

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title = "The nearby field galaxy survey: a spectrophotometric study of 196 galaxies in the local field",

abstract = "The purpose of the present study is to accurately describe the distribution in the local galaxy population of (1) the magnitudes and colors, (2) emission and absorption line strengths, (3) star formation rate and star formation history, (4) morphology, and (5) structural parameters. zie: Chapter 1, introduction",

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N2 - The purpose of the present study is to accurately describe the distribution in the local galaxy population of (1) the magnitudes and colors, (2) emission and absorption line strengths, (3) star formation rate and star formation history, (4) morphology, and (5) structural parameters. zie: Chapter 1, introduction

AB - The purpose of the present study is to accurately describe the distribution in the local galaxy population of (1) the magnitudes and colors, (2) emission and absorption line strengths, (3) star formation rate and star formation history, (4) morphology, and (5) structural parameters. zie: Chapter 1, introduction

KW - Proefschriften (vorm)

KW - Sterrenstelsels

KW - 39.41

M3 - Thesis fully internal (DIV)

SN - 9036713110

PB - s.n.

ER -