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42. http://star.arm.ac.uk/preprints/401.pdf
... C =n CO n kT vT 1 + n a / n cr + 1.5(n a / n cr ) .75 1/2 , (A25) 8kT /(m H2 ) and (A26) (A27) where the mean speed of the molecules vT = n cr = 3.3 в 106 T30 = 3.0 в 10 -16 cm-3 , cm-2 , T3 -1/4 where T 3 T /1000 K. We also have set the average density ...
43. http://star.arm.ac.uk/~ambn/356.pdf
... diameter (m), vi the impactor velocity (m s21) and di the impactor diameter (m ... 106 106 109 109 109 109 20 , V # 25 Min Fraction d (km) prob yr21 10.5 13.2 13.2 13 ... M., Paolicchi P., Farinella P., 1996, Earth, Moon, Planets, 72, 133 Moore H. J ...
44. http://star.arm.ac.uk/preprints/2015/664.pdf
... Planets in the habitable zone of M dwarf stars (0.1 AU from the star) would fare even worse due to their closer proximity, e.g., the 2014 flare of DG CVn produced a radiative flux on such a hypothetical planet 106 times greater than that which the ...
45. http://star.arm.ac.uk/preprints/2010/571a.pdf
... 3-rev Perseid trail; = 0.00025, mean ejection speed = 47/r m/s. Figure 4 Earth's 2009 encounter with 3-rev Perseid trail; = 0.00050, mean ejection speed = 68/r m/s. values are chosen owing to the presumed difference in meteoroid density (Babadzhanov ...
46. References
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