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On the filamentary environment of galaxies

Abstract:

The correlation between the large-scale distribution of galaxies and their spectroscopic properties at z=1.5 is investigated using the Horizon MareNostrum cosmological run. We have extracted a large sample of 10^5 galaxies from this large hydrodynamical simulation featuring standard galaxy formation physics. Spectral synthesis is applied to these single stellar populations to generate spectra and colours for all galaxies. We use the skeleton as a tracer of the cosmic web and study how our g...

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Publication status:
Published

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Journal:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume:
404
Issue:
4
Pages:
1801-1816
Publication date:
2009-10-09
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:0b5f8f9a-9022-4ea5-b23b-7235dea8484a
Source identifiers:
205701
Local pid:
pubs:205701
Language:
English
Keywords:

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