Four Late-type Galaxies with Double Radio Lobes and Properties of Such Galaxies

作     者：Z.S.Yuan X.Y.Gao Z.L.Wen J.L.Han Z.S.Yuan;X.Y.Gao;Z.L.Wen;J.L.Han

作者机构：National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China CAS Key Laboratory of FASTNational Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China School of Astronomy and Space SciencesUniversity of Chinese Academy of SciencesBeijing 100049China 

出 版 物：《Research in Astronomy and Astrophysics》 (天文和天体物理学研究（英文版）)

年 卷 期：2024年第24卷第4期

页      面：84-90页

核心收录：

学科分类：07[理学] 070401[理学-天体物理] 0704[理学-天文学] 

基　　金：partially supported by the National SKA Program of China(grant No.2022SKA0120103) the National Natural Science Foundation of China(Nos.11988101 and 11833009,12073036) support from the science research grants from the China Manned Space Project(CMS-CSST-2021-A01,CMS-CSST-2021-B01) the financial support from the National Key R&D Program of China(No.2021YFA1600401 and 2021YFA1600400) the International Partnership Program of Chinese Academy of Sciences,grant No.114A11KYSB20170044 

主　　题：galaxies:active galaxies:jets galaxies:spiral radio continuum:galaxies 

摘      要：The triggering mechanism for radio lobes from late-type galaxies is not fully *** samples are desired for a thorough investigation and *** utilizing the optical data from the newly released Dark Energy Spectroscopic Instrument imaging surveys and the radio sources from the NRAO VLA Sky Survey and the Faint Images of the Radio Sky at Twenty-centimeter,we identify four Late-type Galaxies with double Radio Lobes(La GRLs):J0217-3645,J0947+6220,J1412+3723 and J1736+*** previously known La GRLs,we confirm the correlation between radio power P_(1.4GHz)and stellar mass M_(*)of host ***(25/35)La GRLs belong to the blue cloud galaxies,while the newly identified cases in this work are located within the region of the red *** find a clear correlation between the differential radio power,i.e.,the offset from the P_(1.4GHz)-M_(*)relation,and the galaxy color,indicating that bluer galaxies at a fixed M_(*)tend to host more powerful radio ***,the majority(31/36)of La GRLs are either located in a galaxy group or displaying a disturbed *** suggest that all of the galaxy mass,color and surrounding environment could play important roles in triggering radio lobes in late-type galaxies.