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31 Jul 2018: radius, and albedo Cont. 3 8.16 9.24 8.67 83 Existence of atmosphere Cont. ... The Messenger 143:16–24. Errmann R, Minardi S, Labadie L, Muthusubramanian B, Dreisow F, NolteS, Pertsch T (2015) Interferometric nulling of four channels with

25 Oct 2018: We also saw in Lecture 2 (eq. 2.24) that in the radiation-dominated era thescale factor of the Universe evolves as a(t) = (t/t0). ... 7. 8. g. 2aT 4 for fermions,. (7.24). in equilibrium when kT mc2.

30 Jul 2018: F7 V 4.126 2.83 2.4 13.7 137 N/– [22, 24, 28]. ... J., Stapelfeldt,K. R., and Wyatt, M. C., “Target Selection for the LBTI Exozodi Key Science Program,” ApJS 216, 24(Feb.

30 Jul 2018: 2 1) (33, 29, 24, 21,. 18, 16, 14 km s1, for planet b to h) for parallel orbits at impactand would be maximal for radial encounters at.

6 Nov 2018: IRJνIRJν. = 2y (10.23). and. y =. kT. mec2σT ne dl (10.24). ... Note that the so-called. Compton y parameter in eq. 10.24 increases with T, since the temperaturedetermines the average energy transfer per scattering event.

13 Nov 2018: 20. 8πGmH(12.16). (Y is the baryonic mass fraction in He: Yp = 0.24) and. ... bT (. 2kT. mH. )1/2= 12.8 T. 1/24 km s. 1 (12.22).

14 Jun 2018: MNRAS 000, 1–21 (2017) Preprint 14 June 2018 Compiled using MNRAS LATEX style file v3.0. Modelling the KIC8462852 light curves: compatibility of the dipsand secular dimming with an exocomet interpretation. M. C. Wyatt1?, R. van Lieshout1, G. M.

20 Jul 2018: 2015);e.g., stars in such regions that do not show evidence of 24 µ m emission above pho-tospheric levels are designated as class III stars (as opposed to class ... I or II starsfor which excess 24 µ m emission is present), and are normally considered

9 Nov 2018: θ λ Depth. 3542116 1268.2 11.0 1.05 0.24 0.23 0.001033542116 991.9 8.3 1.08 0.28 0.25 0.00074. ... For KIC 8027456, assuming M? = 2M, R? = 1.5R?,and θ = 0.24 days yields an upper limit of rt < 1.4au, and acircular period of 1.1 years.

15 May 2018: 1/18 [( rRr0. )7/4 1. ]. (20). The distance-dependent factor in this equation (in square brackets)equals unity at r0/rR = 24/7 0.67 and goes to zero for ... CR2.0. )7/2(ρd. 3 g cm3. )11/18. (25). From Eqs. (24) and (25) we find that the value of ΣR