Issue |
A&A
Volume 442, Number 1, October IV 2005
|
|
---|---|---|
Page(s) | 117 - 124 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20041448 | |
Published online | 30 September 2005 |
The spectral-type/luminosity and the spectral-type/satellite-density relations in the 2dFGRS
1
Dipartimento di Astronomia, Università di Bologna, V. Ranzani 1, 40127 Bologna, Italy e-mail: birgit.kelm@unibo.it
2
INAF – Osservatorio Astronomico di Capodimonte, V. Moiariello 16, 80131 Napoli, Italy
Received:
10
June
2004
Accepted:
19
June
2005
We examine the relative fractions of passive
(type 1), quiet-SF (type 2) and active-SF (type 3+4) galaxies as a function of
luminosity and number of neighbours in several volume-limited samples selected from the 2dFGRS.
Neighbours are counted within 1 Mpc projected distance
and ±1000 km s-1 depth. We apply a maximum magnitude difference
criterion and require neighbours to be fainter than the galaxy itself.
We show that, whatever the environment, passive galaxies dominate in bright samples and active-SF galaxies in faint samples, whereas quiet-SF galaxies
never dominate. We further show that in bright samples (MB – 5
h75 ≤
) the fraction of passive galaxies grows steadily
with fainter neighbour density, whereas in faint samples a threshold-like
dependence is observed. This suggests that the spectral-type/density
(≈morphology/density) relation extends to the intermediate dense
environment, but only in the surroundings of luminous galaxies and that it
reflects an enhancement of the number of satellites rather than stronger
clustering among galaxies themselves. Our analysis indicates that, in general,
luminosity is a good tracer of galaxy halo mass and that it dominates over
environment (satellite density) in setting the spectral type
mix of a population. However, minority populations exist, such as luminous
SF galaxies and faint passive galaxies, whose luminosity is an inaccurate
tracer of halo mass.
Key words: galaxies: general / galaxies: fundamental parameters / galaxies: stellar content / galaxies: statistics / galaxies: clusters: general
© ESO, 2005
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