1. Luminous and dark matter in spiral galaxies Irina Yegorova Fellow Symposium 8-10 June 2009 ESO, Garching Paolo Salucci (SISSA, Italy)‏ Alessandro Pizzella (University of Padova, Italy)‏ Uli Klein (University of Bonn, Germany)‏ Gianfranco Gentile (Sterrenkundig Observatorium, Belgium)‏ Kristine Spekkens (Kingston, Canada)‏

2. Freeman (1970)‏ Properties of Spiral Galaxies Masses ~ 10 9 – 10 12 M M B ~ from -16 to -23 D ~ 5—100 kpc

4. Rotation curves of spiral galaxies NGC 2403 Discrepancy resolved by postulating dark matter Expected v c ~ r  1/2 beyond luminous region

5. The Tully-Fisher (TF) relation is an empirically established correlation between the luminosity L of a spiral galaxy and its rotational velocity V (Tully & Fisher, 1977)‏

6. Physical basis of the TF-relation From the equation of centrifugal equilibrium we get: V 0 – representative velocity, M - total mass, R c – characteristic radius of luminous matter  - structural parameter depending on the shape of the mass distribution

7. The first equation can be written in this form: this equation can be written in the form of the Tully-Fisher relation:

8. Samples: 1 st sample: 967 spiral galaxies Mathewson (1992) 2 nd sample: 304 spiral galaxies Courteau (1997)‏ 86 galaxies selected for analysis 3 sample: 329 spiral galaxies Vogt (2004)‏ 81 galaxies selected for analysis Vmax

9. Radial TF-relation for 967 galaxies

10. Slope and scatter of the RTF-relation

11. Physical meaning of the slope The slope of the TF-relation steadily rises with distance due to the fact that the fractional amount of the dark matter in galaxies changes with the radius.  increases with R this has influence on the slope

12. slope=-7,579; scatter=0.328; N of galaxies=843 slope=-5.54; scatter=0.49; N of galaxies=83 TF-relation using V max

14. Probing dark matter halos of spiral galaxies with their satellites 1.5 - 2 satellites per host galaxy Zaritsky (1993): 45 primaries – 69 satellites Kitt Peak 2.3 m Sales & Lambas (2004): 1498 primaries – 3079 satellites 2dFGRS 3.9 m T. Breinerd (2004) 3 samples: 1351 primaries – 2084 satellites, 948 primaries – 1294 satellites, 400 primaries – 658 satellites SDSS 2.5 m

15. Less primaries  bigger telescope  more satellites late type spirals isolated already known have at least 4 satellites redshift 0.029 < z < 0.085 7 primaries  VLT, VIMOS

16. SDSS J154040.56-000933.5 z=0.078 VIMOS, VLT

17. Candidates for satellites: Found within r < 1000 kpc ∆V < 500 km/s

18. 7 primaries 77 satellites identified 740.038 SDSSJ221957.2 820.077 SDSSJ154904.29 1170.075 SDSSJ154040.5 1950.085 SDSSJ153221.6 1740.083 SDSSJ152621.67 740.046 SDSSJ145211.01 840.029 SDSSJ134215.02 N of sat. (found)‏ N of sat. (SDSS)‏ zPrimary galaxy

19. SDSS J145211.01+044053.6

24. Salucci et al. (2007)‏ 500 kpc

25. Plans: To do the same kind of work for the early-type galaxies