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23 Aug 2018: Age (Myr) DBA 223 41/214 42 235 42/223 43 227 11/216 10 228 20/218 20DBAZ 220 59/213 53 230 65/222 55 223 10/215 10 ... Gänsickeet al. 2016). Taking a minimum of ten orbits for the lifetimeof the transit features implies k > 20 to avoid

18 Oct 2018: 3/20. =. 2. 3H10 (5.20). 5.3 Cosmological Distances. 5.3.1 Proper Distance.

31 Jul 2018: 15. 20. 25. Rea. l,0. 86m. m[m. Jy]. 12m band 7. ... Particles are initially randomly distributed in the sys-tem with a uniform distribution in semi-major axis (a) be-tween 20 and 170 au (i.e.

28 Nov 2018: The two methods have been used togetherfor galaxies with distances d < 20 Mpc, providing important consistencychecks.

30 Jul 2018: For example, CO de-tected at 20 au in η Corvi is inferred to originate in the sublimationof such an exocomet population (Marino et al. ... not exceeding two months). The whole set of 900simulations took 2 months on 20 CPUs, whereas inclined cometswould

22 Nov 2018: In our own Galaxy and M31, the mass of atomic and moleculargas amounts to only 10–20% of the stellar mass. ... 20. eq. 16.44 gives:. µ1,2 =. (1. [θEθ1,2. ]4)1=. u2 2.

2 Apr 2018: 88230 GJ 380 -0.111 0.059 -0.077 0.056 20 -0.189 0.087 13 pix 2.59104 -299 217 -1.4.

18 Jan 2018: n 20. 18Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 18 January 2018 (MN LATEX style file v2.2). ... Acke et al. 2012; MacGregor et al. 2017). For β Pic and HR 4796A, these observations are made atthe 10 to 20 million-year age that places

14 Jun 2018: 2016). This seemingly normal main sequence Fstar was found to exhibit dips in the light-cuve during which thestellar flux dropped by up to 20% in events that lasted from afraction ... 10. wavelength 6 [7m]. uxden. sity. F8;th[m. Jy]. q = 0:04 au, e = 0:90

5 Apr 2018: are derived assuming stars have reached themain-sequence, using tabulated values from Pecaut & Mamajek (2013), for all stars older than 20 Myr except low-mass AUMic, which is still pre-main ... 2015). For stars younger. than 20 Myr, we use values from