http://www.holoscience.com/news/eta_carina.htmA Hubble Space Telescope image of Eta Carina is shown scaled to fit within the much larger X-ray nebula discovered by Chandra. The lobes are as wide as our solar system and expanding in opposite directions away from a central bright disk at speeds in excess of 1 million km/h (600,000 mph). The odd shape is believed to be partly due to the star's intense magnetic field channeling plasma.
"It is not what I expected," said Dr. Fred Seward of the Harvard-Smithsonian Center for Astrophysics. The new X-ray observation shows three distinct structures: an outer, horseshoe-shaped ring about 2 light years in diameter, a hot inner core about 3 light-months in diameter, and a hot central source less than 1 light-month in diameter which may contain the superstar that drives the whole show. The outer ring provides evidence of another large explosion that occurred over 1,000 years ago.
All three structures are thought to represent shock waves produced by matter rushing away from the superstar at supersonic speeds. The temperature of the shock-heated gas ranges from 60 million deg Kelvin in the central regions to 3 million K (108 million deg. F to 5.4 million deg. F) on the outer structure.
Since it looked like a supernova, one naturally would assume that was the end of the star. All that should be left are beautiful nebula and, perhaps, a neutron star or black hole where the original star once stood. Instead, Eta Cannae is still there (in a subtle bit of grammar, astronomers refer to the star as Eta Carinae and the nebula as Eta Carina).