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6 Nov 2023: 11.24). Note that the free-fall timescale is independent of the initial radius of thesphere, and depends only on the initial density ρ0. ... One such evolutionary track is givenapproximately by:. log L = 10 log M 7.24 log Teff C (11.37).

22 Mar 2024: Equations (24)–(27). 4 A. A. SEFILIAN, R. R. RAFIKOV, & M.

22 Mar 2024: MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled usingMNRASLATEXstyle file v3.0. Has the dust clump in the debris disk of Beta Pictoris moved? Y.Han,1 M.C.Wyatt,1 W.R. F.Dent,21Institute of Astronomy, University of Cambridge, Madingley Road

22 Mar 2024: M = H(q)𝑇 N1H(q), (23). j = H𝑇 N1V. (24). Finally, I𝑠 = 𝝁 is used as the inferred brightness. ... 2). (27). This change to H(q) is used in Equations 21–24 or when comput-ing the model visibilities (Equation 18), with the code

20 Feb 2024: 33 obs D 0. 06 max. (24). max = 2. 7 10 27 M 3. ... 67 c D 0. 65 obs. (26) hen comparing equation ( 24 ) with the numerical model fromarino et al. (

29 Sep 2023: 𝑀bb = 1.75 107𝑅13/3bb 𝑡. 1oct𝑀mid, (24). where 𝑀bb and 𝑀mid are in 𝑀, 𝑅bb is the black body radius of thebelt in au and 𝑡oct is in Myr. ... This is why the blackbodyradius is used in equation 24 and the belt mass is correct

24 Nov 2023: 24. and their evolution, Chevalier and collaborators showed that they occurin sheets of dust (and gas) located 120 and 330 pc in front of thesupernova, and that the dust producing the

11 Jul 2023: ṁrv,k = χrk(fv,k)mv,kR. rk. (24). 2.5 Release of CO following collisions.

17 Oct 2023: ARI's TAP access to the Gaia Archive. Unique source identifier (unique within a particular Data Release) Basis function coefficients for the BP spectrum representation Basis function coefficients for the RP spectrum representation