The Structure of Galaxies at Faint Light Levels: Probing Galaxy Assembly
نویسنده
چکیده
Many clues about the galaxy assembly process lurk in the faint outer regions of galaxies. Although quantitative study of these parts has been severely limited in the past, breakthroughs are now being made thanks to the combination of wide-area star counts, deep HST imagery and 8-m class spectroscopy. I highlight here some recent progress made on deciphering the fossil record encoded in the outskirts of our nearest large neighbours, M31 and M33.
منابع مشابه
ar X iv : a st ro - p h / 06 01 12 1 v 1 6 Ja n 20 06 RESOLVING THE STELLAR OUTSKIRTS OF M 31 AND M 33
Many clues about the galaxy assembly process lurk in the faint outer regions of galaxies. The low surface brightnesses of these parts pose a significant challenge for studies of diffuse light, and few robust constraints on galaxy formation models have been derived to date from this technique. Our group has pioneered the use of extremely wide-area star counts to quantitatively address the large-...
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