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The 2dF Galaxy Redshift Survey: Galaxy clustering per spectral type

Abstract:

We have calculated the two-point correlation functions in redshift space, Ζ (σ, π), for galaxies of different spectral types in the 2dF Galaxy Redshift Survey. Using these correlation functions, we are able to estimate values of the linear redshift-space distortion parameter, β ≡ Ωm0.6/b, the pairwise velocity dispersion, a, and the real-space correlation function, Ζ(r), for galaxies with both relatively low star formation rates (for which the present rate of star formation is less than 10 pe...

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Journal:
Monthly Notices of the Royal Astronomical Society
Volume:
344
Issue:
3
Pages:
847-856
Publication date:
2003-09-21
DOI:
ISSN:
0035-8711
URN:
uuid:604bcb0f-492d-498a-a620-f35c575bee2b
Source identifiers:
159700
Local pid:
pubs:159700

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