COSMOLOGICAL DISTANCES, DYNAMICS, AND DISTRIBUTIONS
A journey to H0 and beyond via 6619 spiral galaxies

Mikko Hanski, 2001, PhD thesis, Annales Universitatis Turkuensis, ser. AI, vol. 268
 
Contents
     
  Header 1
1 Introduction 7
  1.1  Basics of modern cosmology 7
  1.2  Galaxies 11
  1.3  Distance scale 12
  1.4  The aim of this thesis 14
2 KLUN galaxy sample 17
3 Tully-Fisher relation, Malmquist bias, and H0 19
  3.1  The Tully-Fisher relation 19
  3.2  The Malmquist bias and the normalized distance method 20
  3.3  Problems with the inverse Tully-Fisher relation 22
  3.4  Is H0 55, 72, or something in between? 23
4 Further applications 25
  4.1  Peculiar velocities in the Perseus-Pisces region 25
  4.2  Luminosity and velocity functions 27
  4.3  Radial space distribution of galaxies 32
5 Conclusion 34
  Bibliography 36
  Papers:  
I Theureau, G., Hanski, M., Teerikorpi, P. et al., 1997, A&A 319, 435  
II Theureau, G., Hanski, M., Ekholm, T. et al., 1997, A&A 322, 730  
III Teerikorpi, P., Hanski, M., Theureau, G. et al., 1998, A&A 334, 395  
IV Teerikorpi, P., Ekholm, T., Hanski, M., Theureau, G., 1999, A&A 343, 713  
V Ekholm, T., Teerikorpi, P., Theureau, G. et al., 1999, A&A 347, 99  
VI Hanski, M.O., Theureau, G., Ekholm, T., Teerikorpi, P., 2001, A&A 378, 345  
VII Hanski, M., 2001, submitted