... Finally, the maximum Rossby number, Ro, is calculated using the following formula: Ro = vT a/(b2 3 f ), of Mitchell et al. the semi-major axis is in units of 106 m and vT is likewise the tangential wind velocity in m s-1 . ...
26. http://www.stsci.edu/~inr/nstarsres/upsand.ps
... S. E. Gesser (Green belt: NASA/GSFC) Hamuy, M., Suntzeff, N. B., Heathcote, S. R., Walker, A. R., Gigoux, P., & Phillips, M. M. 1994, PASP, 106, 566 Henry, T., & McCarthy, D. 1993, AJ, 106, 773 Holman, M., Touma, J., & Tremaine, S. 1997, Nature, 386, 254 ...
27. http://www.stsci.edu/~marel/abstracts/psdir/1999ApJS..124..383C.ps
... dark , !\ 2.5, and with the option of a nuclear BH (' dark \ of mass All these param [GM BH /r) M BH \ 3 ] 106 M _ . ...
28. GHRS Observations of the Extrasolar Protoplanetary System Pictoris
... 1991, A&A, 241, 488 . Beust, H. & Tagger, M. 1993, Icarus 106, 42 . Beust, H. & Morbidelli 1995, Icarus, in press . Beust, H. et al. ...
29. Spectroscopic Analysis of the Wind Lines of the Symbiotic Nova AG Peg
... Kenyon, S.J., Mikolajewska, J., Mikolajewski, M., Polidan, R.S., & Slovak, M.H. 1993, AJ 106, 1573 . ...
30. Ultraviolet Observations of the Dwarf Spheroidal Galaxy Leo I
... Kurucz, R. L. 1979, ApJS, 40, 1 . Lee, M. G., Freedman, W., Mateo, M., Thompson, I., Roth, M., & Ruiz, M.-T. 1993, AJ, 106, 1420 . ...