Galaxy in the constellation Pegasus
NGC 7236 is an interacting lenticular galaxy located in the constellation Pegasus. It is located at a distance of about 300 million light years from Earth, which, given its apparent dimensions, means that NGC 7236 is about 150,000 light years across. NGC 7236 forms a pair with NGC 7237 and is a radio galaxy. It was discovered by Albert Marth on August 25, 1864.
NGC 7236 forms a pair with elliptical galaxy NGC 7237, which lies 35 arcseconds to the southeast. The two galaxies are undergoing a merger and are surrounded by hot gas (corona) with temperature of around 1 keV. The total mass of that gas is estimated to be . A smaller elliptical galaxy, NGC 7237C, lies 38 arcseconds southeast of NGC 7237. A faint tail emanates from NGC 7236. It is included in the "Atlas of Peculiar Galaxies", in the category diffuse counter-tails. A tail is also visible in X-rays. A dust lane runs across the galaxy.
The galaxy pair is a source of radiowaves. The radio emission has a double lobe structure, with filaments, but no jets, while a weak core is identified as the nucleus of NGC 7237. The filaments could be created by the interaction of hot gas with the preexisting radio emitting plasma. Some bright radio sources are visible within the lobes but they could be background active galaxies.
One supernova has been observed in NGC 7236: SN2019krv (typeIa, mag. 18.4).
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