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On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
2017
Astronomy and Astrophysics
(Abridged) In the last decade several massive molecular gas reservoirs were found <100 kpc distance from active galactic nuclei (AGNs), residing in gas-rich companion galaxies. The study of AGN-gas-rich companion systems opens the opportunity to determine whether the stellar mass of massive local galaxies was formed in their host after a merger event or outside of their host galaxy in a close starbursting companion and later incorporated via mergers. We study the quasar-companion galaxy system
doi:10.1051/0004-6361/201628173
fatcat:3aij7ei3gvf2lngsaog4lbvydm