- Abstract:
-
In colour-magnitude diagrams most galaxies fall in either the ``blue cloud'' or the ``red sequence'', with the red sequence extending to significantly brighter magnitudes than the blue cloud. The bright-end of the red sequence comprises elliptical galaxies (Es) with boxy isophotes and luminosity profiles with shallow central cores, while fainter Es have disky isophotes and power-law inner surface-brightness (SB) profiles. An analysis of published data reveals that the centres of galaxies with...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2007.12505.x
-
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- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 382
- Issue:
- 4
- Pages:
- 1481-1493
- Publication date:
- 2007-07-27
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:47c33603-424b-4f64-80ae-9d6131a8340b
- Source identifiers:
-
167405
- Local pid:
- pubs:167405
- Language:
- English
- Keywords:
- Copyright date:
- 2007
- Notes:
-
MNRAS, accepted. Added discussion and references, conclusions
unchanged. 14 pages, 6 figures (2 color)
Journal article
The role of thermal evaporation in galaxy formation
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