Kinematic properties of double-barred galaxies: Simulations versus integral-field observations
Using high-resolution N-body simulations, we recently reported that a dynamically cool inner disk embedded in a hotter outer disk can naturally generate a steady double-barred (S2B) structure. Here we study the kinematics of these S2B simulations, and compare them to integral-field observations from...
Κύριοι συγγραφείς: | , , , |
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Μορφή: | Journal article |
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Institute of Physics
2016
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