Simulations of the Formation and X-ray Emission from Hot Bubbles in Planetary Nebulae
Instituto de Radioastronomía y Astrofísica (IRyA), UNAM Campus Morelia, 58090 Morelia, Michoacan, Mexico
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Received: 26 June 2018 / Revised: 18 July 2018 / Accepted: 23 July 2018 / Published: 30 July 2018
High-quality X-ray observations of planetary nebulae (PNe) have demonstrated that the X-ray-emitting gas in their hot bubbles have temperatures in the small range
= (1 − 3) × 10
K. However, according to theoretical expectations, adiabatically-shocked wind-blown bubbles should have temperatures up to two orders of magnitude higher. Numerical simulations show that instabilities at the interface between the hot bubble and the nebular material form clumps and filaments that generate an intermediate-temperature turbulent mixing layer. We describe the X-ray properties resulting from simulations of PNe in our Galaxy and the Magellanic Clouds.
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MDPI and ACS Style
Toalá, J.A.; Arthur, S.J. Simulations of the Formation and X-ray Emission from Hot Bubbles in Planetary Nebulae. Galaxies 2018, 6, 80.
Toalá JA, Arthur SJ. Simulations of the Formation and X-ray Emission from Hot Bubbles in Planetary Nebulae. Galaxies. 2018; 6(3):80.
Toalá, Jesus A.; Arthur, S. J. 2018. "Simulations of the Formation and X-ray Emission from Hot Bubbles in Planetary Nebulae." Galaxies 6, no. 3: 80.
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