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Trends along the Hubble Sequence☛ Colours : RC2 (de Vaucouleurs et al. 1977),RC3 (Buta(et al. 1995) . . . . . . . . . . . . . . . . . . . . . . . . .

Struktur von Galaxien - Astro F-Praktikum Göttingen

Photometrie eines Sternhaufen - Astro F-Praktikum Göttingen

Local GalaxiesLocal luminosity functions for galaxies :field galaxiesbreak-downinto typesfaint end slope α ~ –1.1(N galgal ➙ inf. . for L B ➘)cluster galaxies:steep faint end slopefaint end slope α

Trends along the Hubble Sequence☛ Colours : RC2 (de Vaucouleurs et al. 1977),RC3 (Buta(et al. 1995) . . . . . . . . . . . . . . . . . . . . . . . . .

Page 1 and 2: The Physics of GalaxiesObservations
Page 5 and 6: Brief History of Galaxy Research☛
Page 8 and 9: Local GalaxiesFerguson+98 : Hα emi
Page 10 and 11: Galaxies beyond the Hubble Sequence
Page 12 and 13: * what the hell is [Fe/H] ?Local Ga
Page 16: Trends along the Hubble Sequence☛

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