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The conformity of HI galaxies in ALFALFA-SDSS sample
作者姓名:Lin-Cheng Li  Bo Qin  Jie Wang  Jing Wang  You-Gang Wang
作者单位:National Astronomical Observatories;School of Astronomy and Space Science;International Centre for Radio Astronomy Research(ICRAR);Department of Astronomy
基金项目:funded by the National Key R&D Program of China(Grant No.2018YFA0404603);supported by CAS Interdisciplinary Innovation Team(JCTD-2019-05)。
摘    要:The conformity effect,indicating the evolution of galaxies is related to its surrounding neighbor 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 H i galaxies as a function of distance around a normal or an H i 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 1010*/M<1010.5.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 investigations.Our results provide another viewpoint on the conformity effect and hope to shed light on the co-evolution of the galaxies and their neighbors in the current galaxy formation models.

关 键 词:method  data  analysis-radio  lines  galaxies-galaxies  evolution

The conformity of HI galaxies in ALFALFA-SDSS sample
Lin-Cheng Li,Bo Qin,Jie Wang,Jing Wang,You-Gang Wang.The conformity of HI galaxies in ALFALFA-SDSS sample[J].Research in Astronomy and Astrophysics,2021(2).
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