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arXiv · astro-ph/0701704

Detection of a Stellar Halo in NGC 4244

Anil Seth·Roelof De Jong·Julianne Dalcanton·the GHOSTS team
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Abstract

We present the preliminary detection of a stellar halo in the nearby, edge-on galaxy, NGC 4244. Using data from the Hubble Space Telescope's Advanced Camera for Surveys (HST/ACS), we have examined number counts of red giant branch (RGB) stars along the minor axis of the galaxy out to 10 kpc, with a limiting surface brightness of mu_R ~ 31 mag/arcsec^2. At distances more than 2.5 kpc above the disk, a second stellar component is clearly visible. This component is well fit by either an exponential or a power law. The best-fit exponential scale height is similar to the scale length of the galaxy disk, suggesting that we are indeed detecting a halo component. Furthermore, the color of the RGB stars above 2.5 kpc are significantly bluer than those in the disk, suggesting a more metal-poor population. Outside the local group, this finding represents one of the first detections of a resolved stellar halo in a spiral galaxy.

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Anil Seth, Roelof De Jong, Julianne Dalcanton, the GHOSTS team. 2007-01-24. Detection of a Stellar Halo in NGC 4244. https://doi.org/10.1017/s1743921307009003

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