X-ray Observations of Planetary Nebulae since WORKPLANS I and Beyond
Planetary nebulae (PNe) were expected to be filled with hot pressurized gas driving their expansion. ROSAT hinted at the presence of diffuse X-ray emission from these hot bubbles and detected the first sources of hard X-ray emission from their central stars, but it was not until the advent of Chandra and XMM-Newton that we became able to study in detail their occurrence and physical properties. Here I review the progress in the X-ray observations of PNe since the first WORKshop for PLAnetary Nebulae observationS (WORKPLANS) and present the perspective for future X-ray missions with particular emphasis on eROSITA.
2006 ◽
Vol 368
(4)
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pp. 1706-1716
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2010 ◽
Vol 721
(2)
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pp. 1820-1828
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