Study of recent outburst in the Be/X-ray binary RX J0209.6-7427 with AstroSat: a new ultralurninous X-ray pulsar in the Magellanic Bridge?

We present the timing and spectral studies of RX J0209.6-7427 during its rare 2019 outburst using observations with the Soft X-ray Telescope (SXT) and Large Area X-ray Proportional Counter (LAXPC) instruments on the AstroSat satellite, Pulsations having a periodicity of 9.29 s were detected for the first time by the NICER mission in the 0.2-10 keV energy band and, as reported here, by AstroSat over a broad energy band covering 0.3-80 keV. The pulsar exhibits a rapid spin -up during the outburst. Energy resolved folded pulse profiles are generated in several energy bands in 3-80 keV. To the best of our knowledge this is the first report of the timing and spectral characteristics of this Be binary pulsar in hard X-rays, There is suggestion of evolution of the pulse profile with energy, The energy spectrum of the pulsar is determined and from the best-fitting spectral values, the X-ray luminosity of RX J0209.6-7427 is inferred to be 1,6 x 1039 erg Our timing and spectral studies suggest that this source has features of an ultraltiminous X-ray pulsar in the Magellanic Bridge, Details of the results are presented and discussed in-terms of the current ideas.