Tracing the outer halo in a giant elliptical to 25 Reff
M. Rejkuba, W. E. Harris, L. Greggio, G. L. H. Harris, H. Jerjen, O., A. Gonzalez

TL;DR
This study uses HST imaging to resolve individual stars in the halo of NGC 5128, revealing its structure, metallicity gradient, and star distribution out to 25 effective radii, providing detailed insights into its outer halo properties.
Contribution
First detailed mapping of stellar populations and metallicity gradients in the outer halo of a giant elliptical galaxy out to 25 Reff using resolved star observations.
Findings
Halo is more elongated along the major axis.
Metallicity decreases smoothly with radius.
Outer halo follows a power-law density profile.
Abstract
We have used the ACS and WFC3 cameras on board HST to resolve stars in the halo of the nearest giant elliptical (gE) galaxy NGC 5128 out to a projected distance of 140 kpc (25 effective radii, Reff) along the major axis and 90 kpc (16 Reff) along the minor axis. This dataset provides an unprecedented radial coverage of the stellar halo properties in any gE galaxy. Color-magnitude diagrams clearly reveal the presence of the red giant branch stars belonging to the halo of NGC 5128, even in our most distant fields. The star counts demonstrate increasing flattening of the outer halo, which is elongated along the major axis of the galaxy. The V-I colors of the red giants enable us to measure the metallicity distribution in each field and so map the gradient out to ~16 Reff from the galaxy center along the major axis. A median metallicity is obtained even for the outermost fields along both…
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