Models of our Galaxy II
Stars near the Sun oscillate both horizontally and vertically. In Paper I the coupling between these motions was modelled by determining the horizontal motion without reference to the vertical motion, and recovering the coupling by assuming that the vertical action is adiabatically conserved as the...
| मुख्य लेखकों: | , |
|---|---|
| स्वरूप: | Journal article |
| प्रकाशित: |
2011
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