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Katsuda, S., Acero, F., Tominaga, N., Fukui, Y., Hiraga, J.S., Koyama, K., Lee, S.H., Mori, K., Nagataki, S., Ohira, Y., Petre, R., Sano, H., Takeuchi, Y., Tamagawa, T., Tsuji, N., Tsunemi, H. and Uchiyama, Y. (2015) Evidence for Thermal X-Ray Line Emission from the Synchrotron-Dominated Supernova Remnant RX J1713.7-3946. The Astrophysical Journal, 814, 29.

has been cited by the following article:

• TITLE: The Fermi Bubbles as a Superbubble

  AUTHORS: Lorenzo Zaninetti

  KEYWORDS: ISM, Bubbles, ISM, Clouds, Galaxy, Disk, Galaxies, Starburst

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.8 No.2, June 22, 2018

  ABSTRACT: In order to model the Fermi bubbles we apply the theory of the superbubble (SB). A thermal model and a self-gravitating model are reviewed. We introduce a third model based on the momentum conservation of a thin layer which propagates in a medium with an inverse square dependence for the density. A comparison has been made between the sections of the three models and the section of an observed map of the Fermi bubbles. An analytical law for the SB expansion as a function of the time and polar angle is deduced. We derive a new analytical result for the image formation of the Fermi bubbles in an elliptical framework.