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Symposium 241
Symposium 241
Abstract details
The Stellar Structures around Disk Galaxies
Igor Drozdovsky, Antonio Aparicio, Carme Gallart, Matteo Monelli, Sebastian Hidalgo, Eduard Bernard, Nikolay Tikhonov, Olga GalazutdinovaAbstract
I'll present a summary of our systematic and homogeneous analysis of the
surface number counts and population gradients of the resolved stars in
surroundings of the nearby disk galaxies, observed with space- (Hubble &
Spitzer) and ground-based telescopes. We examine the radial (in-plane)
and vertical (extraplanar) distributions as a function of stellar age by
tracking changes in the color-magnitude diagram of face-on and edge-on
galaxies. In particular, I will focus on our recent extensive study of
three Local Group disk galaxies, IC1613, NGC6822 and IC10. Our data show
that the scale length and height of a stellar population increases with
age, with oldest of the detected red giant branch population (RGB)
identified at large galactocentric radii or extraplanar height, out to
typically a few kpc. In the most massive of the studied galaxies there
is evidence for a break in number density and color gradients of evolved
RGB stars, which plausibly correspond to the thick disk and halo
components of the galaxies. The results may imply that all massive
spiral galaxies not only have a thick disk but also poses an extended
halo, while dwarf disk galaxies have solely a thin/thick disk component.
When complemented with detailed chemical abundance and kinematic
information from spectra of these stars, our optical/near-IR
photometric data will allow us to shed light on fundamental questions
about the evolution of disk galaxies, such as disk heating versus merger
scenarios and a role of these mechanisms in forming the stellar disks
and halo.