Parameterizations of a galaxy's gravitational potential introduced by Miyamoto and Nagai (1975).
From
Since Poisson's equation is linear, another pair of potentials is obtained by differentiating (3) and (1) n times with respect to b] . As
,
where
(1)
From
(2)
(3)
Since Poisson's equation is linear, another pair of potentials is obtained by differentiating (3) and (1) n times with respect to b] . As
,(4)
(5)
where
(6)
回复Comments
{commenttime}{commentauthor}
{CommentUrl}
{commentcontent}