111. CHIANTI atomic database
... D.H., Fontes, C.J., 1990, ADNDT, 44, 31 %oscillator strengths: Martin, I., Karwowski, J., Diercksen, G.H.F., Barrientos, C., 1993, A , 100, 595 %oscillator strengths: Wiese, W.L., Smith, M.W., Glennon, B.M., 1966, Atomic Transition Probabilities, NSRDS ...
112. http://www.arcetri.astro.it/~lt/preprints/ngc2346/ngc2346.ps.gz
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113. CHIANTI atomic database
... 31, 506 %A values (1-3, 2-phot): Drake, G.W.F., Phys Rev A, 1986, 34, 2871 %oscillator strengths: Wiese,W.L., Smith,M.W., Glennon,B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4 %comment: Wiese's oscillator strengths are hydrogenic %produced as ...
114. http://www.arcetri.astro.it/irlab/doc/library/AOA/APNDXC.PDF
... Z X C V B N M Down 1A 1B 1C 1D 1E 1F 20 21 22 23 24 25 26 27 28 29 2A 2B 2C 2D 2E 2F 30 31 32 Up 9A 9B 9C 9D 9E 9F A0 A1 A2 A3 A4 A5 A6 A7 A8 A9 AA AB AC AD AE AF B0 B1 B2 Key ,< .> ...
115. http://www.arcetri.astro.it/science/chianti/chianti_3.03/elements/fe/fe_22.html
... agree with NIST observed wavelength on the order of 1- 10% %oscillator strengths(16- 125): Sampson, D. H., Weaver, G. M., Goett, S. J., Zhang, H., Clark, R. E. H., ADANDT, 44,31 (1990). %energy levels: J. Sugar and C. Corliss, 1985, J. Phys. Chem ...
116. CHIANTI atomic database
... agree with NIST observed wavelength on the order of 1- 10% %oscillator strengths(16- 125): Sampson, D.H., Weaver, G.M., Goett, S.J., Zhang, H., Clark, R.E.H., 1990, ADNDT, 44, 31 %A values (above IP): calculations of Safronova reported in Kato et al ...
117. http://www.arcetri.astro.it/irlab/doc/library/intel/24369101.pdf
... 31 25 24 23 22-18 17 16 15 14 13 12 11 10 09 08 07 06 05 04 03 02 01 00 F X S R M M X Reserved (0) rsvd PP SA ET 3 6 CMP MCG ... 31 Reserved (set to 0) 10 09 08 07 06 05 PAE 04 PSE 03 DE 02 TSD 01 PVI 00 VME OSFXSR PCE P G E M CE Figure 10-3. ...
118. Appunti Linux: Orologio di sistema e calendario
... 31. Orologio di sistema e calendario . 31.1 Orario locale . ... 31.1 Orario locale . 31.2 Distinzione tra hardware e software . ... 31.2 Distinzione tra hardware e software . 31.2.1 Orologio hardware . ...
119. http://www.arcetri.astro.it/science/starform/preprints/mosca_06.pdf
... This stellar mass can be divided by the total mass of the associated molecular 31 clump, 3 в 103 M (see Section 4.4), to calculate the star formation efficiency, 17%67%. ...
120. Sperello
... of nearby galaxies in the Herschel Reference Survey", L. Ciesla et al. 2010, in "SF2A-2010: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics", S. Boissier, M. Heydari-Malayeri, R. Samadi and D. Valls-Gabaud, eds., p.31 ...