The photometric properties of a vast stellar substructure in the outskirts of M33
We have surveyed approximately 40 deg2 surrounding M33 with Canada-France-Hawaii Telescope MegaCam/MegaPrime in the g and i filters out to a maximum projected radius from this galaxy of 50 kpc, as part of the Pan-Andromeda Archaeological Survey (PAndAS).
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|Source:||Astrophysical Journal Letters|
|01_McConnachie_The_photometric_properties_of_2010.pdf||1.15 MB||Adobe PDF||Request a copy|
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