Search

15 Jan 2015: δE Gm (1 β)2ap. (1 2) , (24). and equating the two energies yields. ... 3. Allow-ing for capture into lower j resonances, the overall captureprobability into the 6:5 mean motion resonance for particleswith similar initial conditions is 0.24.

15 Jan 2015: around 24”, while in the SW wing it is present from 1” to 5”; not only is the emission more. ... 24 –. Disk Spine Position: Observations and Models. -200 -100 0 100 200Distance [au].

16 Jun 2015: 5.5.2 SAM Code GOTOBUTTON _Toc361307169 PAGEREF _Toc361307169 24. 5.5.3 Transputer GOTOBUTTON _Toc361307170 PAGEREF _Toc361307170 24. ... 5.5.4 Data Output Format GOTOBUTTON _Toc361307171 PAGEREF _Toc361307171 24. 5.6 Computer Interface GOTOBUTTON

15 Jan 2015: arX. iv:1. 412. 0675. v1 [. astr. o-ph. EP. ] 1. Dec. 201. 4DRAF T VERS IONDECEMBER 3, 2014Preprint typeset using LATEX style emulateapj v. 5/2/11. EXO-ZODI MODELLING FOR THE LARGE BINOCULAR TELESCOPE INTERFEROMETER. GRANT M. K ENNEDY1, M ARK C.

16 Jun 2015: arX. iv:1. 506. 0456. 4v1. [ast. ro-p. h.E. P]. 15 J. un 2. 015. Astronomy & Astrophysicsmanuscript no. AUMic c ESO 2015June 16, 2015. Collisional modelling of the AU Microscopii debris discCh. Schüppler1, T. Löhne1, A. V. Krivov 1, S. Ertel2,

16 Jun 2015: CIRSI gives a whole time on one fill of liquid nitrogen in excess of 30 hours in downward looking mode and approximately 24 hours in upward looking mode.

16 Jun 2015: 9.18 12351.9 68.99 48.9 12400.8 16.89 100 Some contamination. 9.24 12423.7 37.60 58.8 12482.5 7.88 100 Some contamination.