Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-02T19:52:17.419Z Has data issue: false hasContentIssue false
  • English
  • Français

Detection of a stellar halo in NGC 4244

Published online by Cambridge University Press:  01 December 2006

A. Seth ,
R. de Jong  and
J. Dalcanton
A. Seth
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02139 email: [email protected]
R. de Jong
Affiliation:
Space Telescope Science Institute
J. Dalcanton
Affiliation:
University of Washington
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 μR ∼ 31 mag/arcsec2. 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.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 523 - 524
Copyright
Copyright © International Astronomical Union 2007

References

Bullock, J. S., & Johnston, K. V. 2005, ApJ, 635, 931CrossRefGoogle Scholar
Fry, A. M., Morrison, H. L., Harding, P., & Boroson, T. A. 1999, AJ, 118, 1209CrossRefGoogle Scholar
Kalirai, J. S. et al. , 2006, ApJ, 648, 389CrossRefGoogle Scholar
McConnachie, A. W. et al. , 2006, ApJL, 647, L25CrossRefGoogle Scholar
Seth, A. C., Dalcanton, J. J., & de Jong, R. S. 2005a, AJ, 129, 1331CrossRefGoogle Scholar
Seth, A. C. 2005b, AJ, 130, 1574CrossRefGoogle Scholar
Zibetti, S., White, S. D. M., & Brinkmann, J. 2004, MNRAS, 347, 556CrossRefGoogle Scholar