... at far-infrared wavelengths, employing the 63-Іm [O I] line, are presented ... The prominent [O I] 63-Іm emission line may then be due to oxygen release and ... Predictions for the prominent 63-Іm oxygen fine-structure line are displayed in Fig. ...
... 0.67 0.54 1.39 OH 0.17 0.01 0.01 O I 63m > 0.21 1.72 21.36 C I 370m { 0 0.17 the ... 4.76 L and z > 4.36 L. The [O I] 63m line is potentially a good shock diagnostic ...
... Polarisation phase curves for a superfine powder of SiO2 before and after compressing with alcohol drying at = 0.63 µm (left panel) and for size-separated Al2 O3 powders at = 0.63 µm(right panel). ...
... measure the flux at 0.63, 1.0, 1.58, 2.51, 3.98, 6.31 в 10-19 W m-2 arcsec-2 ... S(3) 34 63 no det. no det. 7.3 no det. no det. 4.0 3.3 9.1 20.6 5.1 27.9 2.14µm Cont ...
... A29) Oxygen cooling through 63µm structure line been included in steady shock model intend to include further simulations a convenient largescale dynamical computations molecular turbulence. omit calculation upper energy level generates much weaker 146 ...
... of molecular hydrogen follows the Shapiro & Kang (1987) modifications to the Lepp & Shull (1983) form: 7 Oxygen cooling through the 63-µm fine structure line has been included in the steady shock model and we intend to include it in further simulations in ...
... years of Hirayama Asteroid Families (Y. Kozai, R. P. Binzel and T. Hirayama, eds.) Astronomical Society of Pacific Conference Series, vol. 63, p. 77 Gaffey M.J., Burbine T.H., Binzel R.P., 1993, Meteoritics 28, 161 Hardorp J., 1978, A&A 63, 383 Hardorp J ...