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      https://www.ias.ac.in/article/fulltext/joaa/039/01/0008

    • Keywords

       

      Galaxy merger—dual AGN—radio observations.

    • Abstract

       

      Binary or dual active galactic nuclei (DAGN) are expected from galaxy formation theories. However, confirmed DAGN are rare and finding these systems has proved to be challenging. Recent systematic searches for DAGN using double-peaked emission lines have yielded several new detections, as have the studiesof samples of merging galaxies. In this paper, we present an updated list of DAGN compiled from published data. We also present preliminary results from our ongoing Expanded Very Large Array (EVLA) radio study of eight double-peaked emission-line AGN (DPAGN). One of the sample galaxy shows an S-shaped radio jet. Using new and archival data, we have successfully fitted a precessing jet model to this radio source. We find that the jet precession could be due to a binary AGN with a super-massive black-hole (SMBH) separation of $\sim$0.02 pc or a single AGN with a tilted accretion disk. We have found that another sample galaxy, which is undergoing a merger, has two radio cores with a projected separation of 5.6 kpc. We discuss the preliminaryresults from our radio study.

    • Author Affiliations

       

      K. RUBINUR1 2 M. DAS1 P. KHARB3

      1. Indian Institute of Astrophysics, Bangalore 560 034, India.
      2. Pondicherry University, R. Venkataraman Nagar, Kalapet 605 014, India.
      3. National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, S. P. Pune University Campus, Ganeshkhind, Post Bag 3, Pune 411 007, India.
    • Dates

       
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