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An image of the giant lobes of the planetary nebula KjPn 8 in the light of the emission lines of hydrogen and singly ionised nitrogen, obtained with the narrowband camera on the new 2.3-m Aristarchos telescope. Detailed measurements of the lobes have allowed the determination of their expansion velocity, distance and ages. The results indicate their origin in a remarkable eruptive binary system.
Credit: P. Boumis / J. Meaburn
In the 1950s the planetary nebula KjPn8 was discovered on Palomar Observatory Sky Survey plates. Follow up work in the 1990s by Mexican astronomers at the San Pedro Martir Observatory led to the discovery of giant lobes around the system, one quarter of a degree across, while in 2000 the central star was finally revealed by the Hubble Space Telescope.
An image of the enclosure of the new 2.3-m Aristarchos telescope, sited at Helmos Observatory.
By measuring the velocity and increasing size of the expanding material, the two scientists were able to deduce the distance to the system and date the history of the three ejected lobes. They found that KjPn8 is around 6000 light years away and that the material was thrown out in three phases 3200, 7200 and 50000 years ago.
The inner lobe of material is expanding at 334 km per second, suggesting it originates in an Intermediate Luminosity Optical Transient (ILOT) event. ILOTs are caused by the transfer of material from a massive star to its less massive companion, in turn creating jets that flow in different directions. Boumis and Meaburn believe that the core of KjPn8 is therefore a binary system, where every so often ILOT events lead to the ejection of material at high speed.
Dr Boumis is delighted to see the first results from the new telescope giving clues to the history of such an intriguing system. He comments: “Greece is one of the global birthplaces of astronomy, so it is fitting that research into the wider universe continues in the 21st century. With the new telescope we expect to contribute to that global effort for many years to come.”
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