... e E 1, p E 1, i E 1, 2e E 2, E 2, M 1, M 1, f f f f Selection rule violation no S = 0 quantum numb er change of two(three) electrons no S = 0 no transition b etween levels of different terms Aki 107 102 106 (s-1 ) - 109 - 104 - 108 102 -1 10 -1 1- 10-4 1 ...
[
Текст
]
Ссылки http://www.astro.spbu.ru/staff/afk/AtDatCentre/AtDatCat/Chapter1.pdf -- 64.7 Кб -- 19.11.2010 Похожие документы
... 105. "Thermomagnetic instability in hot discs" . Liverts E., Mond M., Urpin V. MNRAS (accepted December 2010) . 106. ... Liverts E., Mond M., Urpin V. MNRAS (accepted December 2010) . 106. "The nature of optical and near-infrared variability of . ...
... Weil M.L., Hernquist L. Segregation of gas and stars in shell galaxies, 1993, ApJ, 405, 142 . ... Buta R., Crocker D.A. The strange 'barred' spiral galaxy ESO 235-58 - A case of morphological deception, 1993, AJ, 106, 939 . ...
... galaxies (> 106 ): Sky surveys 2dF and 6dF Sky surveys 2dF and 6dF The 2dF (2 degree Field Galaxy Redshift Survey, or 2dFGRS) represents a spectroscopic survey of 5% (2000 sq. deg.) of the sky performed by British and Australian astronomers with the 3.9-m ...
... of C/1995 O1 Hale-Bopp from 13 to 4 AU , by M.Fulle, AJ , 116 , 1470-1477, 1998 ... IR observation of comets by COBE , by C.M.Lisse, AJ , 496 , 971-991, 1998. ... profile in Halley's inner coma , by B.Goidet-Devel, Icarus , 126 , 78-106, 1997 ...
... photometry is the calibrated surface brightness distribution, I (x, y ), in units of m / , in the form of a digital data array ... It consists of a huge amount of numbers ( 106 - 107 ), which do not allow any easy physical interpretation. ...