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Environmental dependence of stellar velocity dispersion in the Main galaxy sample of SDSS DR10

100%
Deng X.-F.
Open Physics
|
2015
|
vol. 13
|
issue 1
EN
The aim of this work is to examine the environmental dependence of stellar velocity dispersion in local galaxies. In studies that likely suffer from the radial selection effect, one has a preference for the use of volumelimited samples. Two volume-limited samples with different redshift and luminosity ranges were constructed from the Main galaxy data of the Sloan Digital Sky Survey Data Release 10 (SDSS DR10). Considering some drawbacks of volume-limited samples, the apparent magnitude-limited Main galaxy sample was also applied. Statistical analyses in these different galaxy samples can reach the same conclusion: galaxies with large stellar velocity dispersions exist preferentially in high density regimes, while galaxies with small stellar velocity dispersions are located preferentially in low density regions, which is inconsistent with that obtained at intermediate redshifts.
2
Content available remote

Compact groups of galaxies (CGs) from the SDSS Data Release 6

45%
Deng X.-F., He J.-Z., Ma X.-s., Jiang P., Tang X.-X.
Open Physics
|
2008
|
vol. 6
|
issue 2
185-193
EN
From the volume-limited MAIN galaxy sample of the SDSS Data Release 6 (SDSS6), we have identified 1298 compact groups of galaxies (CGs) at the neighbourhood radius of R = 1.2 Mpc by three-dimensional cluster analysis. In order to compile the CG catalog, we also estimated velocity dispersion, virial radius, virial mass and crossing time of CGs. In addition, our results show that properties of galaxies may not correlate with merging frequencies.
3
Content available remote

Age-density relation of Main galaxies at fixed parameters or for different galaxy families

45%
Deng X.-F., Song J., Chen Y.-Q., Jiang P., Ding Y.-P.
Open Physics
|
2015
|
vol. 13
|
issue 1
EN
Using two volume-limited Main galaxy samples of the Sloan Digital Sky Survey Data Release 10 (SDSS DR10), we examine the environmental dependence of galaxy age at fixed parameters or for different galaxy families. Statistical results show that the environmental dependence of galaxy age is stronger for late type galaxies, but can be still observed for the early types: the age of galaxies in the densest regime is preferentially older than that in the lowest density regime with the same morphological type. We also find that the environmental dependence of galaxy age for red galaxies and Low Stellar Mass (LSM) galaxies is stronger, while the one for blue galaxies and High Stellar Mass ( HSM ) galaxies is very weak.
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