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20 Nov 2023: cos φm = A Be2, (12). and A and B are functions of a/aN that should be determined. ... φ̈ = (A B cos φ) sin φ, (19). where A and B are functions of the orbital parameters of the particle and satellite that should be determined.

29 Sep 2023: b) Starting from M = E e sin E, r = a(1 e cos E) and h = na2. ... cos g =(1 ra) e. 2. e(1 ra) e, (6). and so that cos g = cos M O(e2).

28 Jun 2020: θ = H0 η (m,0 1)1/2 (15.2). 3. whereby:r(θ) = A(1 cos θ) (15.3). ... m,0 1(15.7). and, more generally,r. rmax=. 1. 2(1 cos θ). (15.8).

6 Dec 2004: a. xx. =. Acos. 2. θBsin. 2. θ. a. yy. =. Asin. 2. θBcos. 2. θ. a. xy. =. 2(A-B)cosθsinθ. where A=1/a. ... 2. and B=1/b. 2. (a and b being the semi-major and semi-minor axes respectively).

6 Dec 2004: a. xx. =. Acos. 2. θBsin. 2. θ. a. yy. =. Asin. 2. θBcos. 2. θ. a. xy. =. 2(A-B)cosθsinθ. where A=1/a. ... 2. and B=1/b. 2. (a and b being the semi-major and semi-minor axes respectively).

22 Nov 2018: systemic velocity of the galaxyindicated by the Doppler shift of the nucleus, and b/a = cos i is the ratioof the minor to the major axis of the ellipse that a ... Right : The observer sees distorted, correlated, images of the distant galaxies.The

22 Mar 2024: to 20 Micron Spectrum of the Planetary-Mass Companion VHS 1256-1257 b. ... JWST Observations of VHS 1256 b 7. calculate a mean image to mitigate the effects of cos-.

14 Feb 2019: 4 becomes. L(θ) cos θσ2i. π/2θ. ie i2. 2σ2i. i2 θ2. ... A simple transformation between. reference frames shows that. cos(dI) = cos(Ib) cos(Ip) sin(Ib) sin(Ip) cos(p b).(9).

22 Mar 2024: b(m)s (α) =2. π. π0. cos(mθ)[1 α2 2α cos θ. ]sdθ, (4). ... B(m)s (α, H) =2. π. π0. cos(mθ). [1α22α cos θH2(1α2). ]sdθ,.

19 Apr 2006: cos. ; ð13Þ. where apl=a, and fs;1, fd, and fi are coefficients corre-sponding to the secular, resonant direct, and resonant indi-rect parts of the disturbing function, respectively. ... The result is. cosm2 : 1. 0:39 0:061=e ; ð26Þ. and these lines