The conformity of HI galaxies in ALFALFA-SDSS sample
Abstract
The conformity effect, indicating the evolution of a galaxy is related to its surrounding neighbour galaxies as far as a few Mpc, is an interesting phenomenon in the modeling of galaxy and evolution. Here we study the conformity effect of HI galaxies in a matched galaxy sample between SDSS DR7 and ALFALFA surveys. By checking the probability difference for the detected HI galaxies as a function of distance around a normal or an HI galaxy, we find that this effect is significant out to 5 Mpc. It also shows a dependence on the stellar mass of galaxies, with the strength the strongest in the stellar mass range of 10^10~10^10.5. However, when the sample is confined to central galaxies in groups with virial radii smaller than 1 Mpc, the 1-halo conformity signal is still evident, while the 2-halo conformity signal is reduced to a very weak amplitude. Our results confirm the previous study in the optical band that the 2-halo term is possibly caused by the bias effect in the sample selection. Furthermore, we confirm the existence of the 1-halo conformity discovered in the optical and radio band in previous lectures. Our results provide another viewpoint of the conformity effect and hope to shed the light on the co-evolution of the galaxies and their neighbours in the current galaxy formation models.
Keywords
Cite
@article{arxiv.2008.05682,
title = {The conformity of HI galaxies in ALFALFA-SDSS sample},
author = {Lincheng Li and Bo Qin and Jie Wang and Jing Wang and Yougang Wang},
journal= {arXiv preprint arXiv:2008.05682},
year = {2021}
}
Comments
11 pages, 6 figures, accepted by Research in Astronomy and Astrophysics