NVSS J161541+221629 , the SIMBAD biblio

The fast-rising blue optical transient AT2018cow indicated unusual early-phase characteristics unlike relatively better studied explosive transients. Its afterglow may be produced by either a relativistically beamed (jetted) or intrinsically luminous (nonjetted) ejecta and carries observational signatures of the progenitor and environment. High-resolution monitoring can distinguish between these scenarios and clarify the progenitor nature. We present very long baseline interferometry (VLBI) observations of AT2018cow at 5 GHz involving 21 radio telescopes from the European VLBI Network with five sessions spanning ≃1 yr. With an astrometric precision up to 25 µas per epoch, the rapidly fading compact mas-scale source is found to be nonjetted with a proper motion of <=0.15 mas yr^–1 (0.14 c). This and a dense (number density ≃10⁴-10⁵ cm^–3) magnetized environment (magnetic field strength >=0.84 G) are characteristic of a newly formed magnetar driven central engine, originating in the successful explosion of a low-mass star.