kw.\*:("TRANSITION ATOMIQUE")
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COMPUTATION OF OSCILLATOR STRENGTHS BY A SEMI-EMPIRICAL METHOD FOR SOME ELEMENTS OF THE IRON GROUP AND THEIR SOLAR PHOTOSPHERIC ABUNDANCE. II. RESULTS FOR SC I.BIEMONT E.1974; SOLAR PHYS.; NETHERL.; DA. 1974; VOL. 39; NO 2; PP. 305-308; BIBL. 19 REF.Article
ANOMALOUS ELECTRON IMPACT EXCITATION OF CA+TULLY JA; PETRINI D; BELY O et al.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 23; NO 1; PP. 15-17; BIBL. 11REF.Serial Issue
THE SQUARE OF THE RADIAL INTEGRAL FOR CALCULATING THE DIPOLE OSCILLATOR STRENGTHS FOR TRANSITIONS IN HYDROGEN ATOMS IN THEIR 3(S, P, OR D) AND 4(S, P, D, OR F) STATESKHANDELWAL GS; FITCHARD EE.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 173; NO 3, PART 1; PP. 737-740; BIBL. 9 REF.Serial Issue
ARC MEASUREMENTS OF FE I OSCILLATOR STRENGTHS.BRIDGES JM; KORNBLITH RL.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 192; NO 3 PART. 1; PP. 793-812; BIBL. 29 REF.Article
NUMERICAL CALCULATIONS OF ATOMIC STRUCTURE CONSTANTS. II. RADIAL PARTS, ENERGY LEVELS, TRANSITION PROBABILITIES FOR FE XIII1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 25; NO 3; PP. 431-435; BIBL. 21REF.Serial Issue
L'UNITE DE TEMPS. SA REALISATION, SON USAGE.GUINOT B.1975; BULL. INFORM. BUR. NATION. METROL.; FR.; DA. 1975; VOL. 6; NO 20; PP. 21-24; ABS. ANGLArticle
COMPUTATION OF OSCILLATOR STRENGTHS BY A SEMI-EMPIRICAL METHOD FOR SOME ELEMENTS OF THE IRON-GROUP AND THEIR SOLAR PHOTOSPHERIC ABUNDANCE. I. RESULTS FOR TI I.BIEMONT E.1974; SOLAR PHYS.; NETHERL.; DA. 1974; VOL. 38; NO 1; PP. 15-31; BIBL. 1 P. 1/2Article
MICROWAVE SPECTRUM OF 13C METHANOL.HAQUE SS; LEES RM; SAIN CLAIR JM et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 187; NO 1 PART. 2; PP. 15-17; BIBL. 12 REF.Article
FURTHER IRON-LINE OBSERVATIONS DURING SOLAR FLARESDOSCHEK GA; MEEKINS JF; COWAN RD et al.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 177; NO 1, PART 1; PP. 261-269; BIBL. 29 REF.Serial Issue
POSSIBILITES DE DETERMINER LA VALEUR DU CHAMP MAGNETIQUE PRES DES PULSARS PAR LA DETECTION DE LA FREQUENCE DE BATTEMENT DANS LES TRANSITIONS ATOMIQUESRUZMAJKIN AA.1975; ASTR. ZH.; S.S.S.R.; DA. 1975; VOL. 52; NO 6; PP. 1173-1177; ABS. ANGL.; BIBL. 7 REF.Article
MULTIPLET SPLITTINGS AND 1S0-3P1 INTERCOMBINATION-LINE OSCILLATOR STRENGTHS IN BE I AND MG I.LAUGHLIN C; VICTOR GA.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 192; NO NO PART. 1; PP. 551-556; BIBL. 22 REF.Article
A THEORETICAL AND EXPERIMENTAL STUDY OF FE XIX TO FE XXIV SOLAR-FLARE SPECTRA AND ISOELECTRONIC SPECTRA IN SULFUR.FAWCETT BC; COWAN RD; HAYES RW et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 187; NO 2 PART. 1; PP. 377-383; BIBL. 20 REF.Article
OSCILLATOR STRENGTHS IN THE TIO ALPHA-BAND SYSTEM.FAIRBAIRN AR; WOLNIK SJ; BERTHEL RO et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 1 PART. 1; PP. 273-277; BIBL. 23 REF.Article
SOME TRANSITIONS OF NE VIII AND AR VIII BETWEEN LEVELS OF PRINCIPAL QUANTUM NUMBERS 3, 4 AND 5DRUETTA M; DATLA RU; KUNZE HJ et al.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 174; NO 1 PART 1; PP. 215-217; BIBL. 11REF.Serial Issue
ATOMIC PROCESSES IN ASTROPHYSICAL PLASMAS.MYERSCOUGH VP; PEACH G.1972; CASE STUD. ATOM. PHYS.; NETHERL.; DA. 1972; VOL. 2; PP. 293-397; BIBL. 343 REF.Article
BEHAVIOR OF DECAYING STATES IN APPLIED FIELDSLOW FE.1979; PHYSICA A; NLD; DA. 1979; VOL. 96; NO 1-2; PP. 260-262Article
APPROXIMATIONS FOR COLLISIONAL AND RADIATIVE TRANSITION RATES IN ATOMIC HYDROGENJOHNSON LC.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 174; NO 1 PART 1; PP. 227-236; BIBL. 37REF.Serial Issue
OSCILLATOR STRENGTHS FOR NEUTRAL SODIUM AND THE INTERSTELLAR SODIUM ABUNDANCE IN ZETA OPHIUCHI.ERMAN P; BRZOZOWSKI J; SMITH WH et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 192; NO 1 PART. 1; PP. 59-62; BIBL. 10 REF.Article
SEMIEMPIRICAL CALCULATION OF GF VALUES. II. FEI (3D+4S)8-(3D+4S)74P.KURUCZ RL.1974; SMITHSON. ASTROPHYS. OBS. SPEC. REP.; U.S.A.; DA. 1974; NO 359; PP. (147P.); ABS. FR. RUSSE; BIBL. 2 P.Article
LIFETIME MEASUREMENTS OF SOME LEVELS OF SMI BY USE OF DYE LASER EXCITATIONMAREK J; MUENSTER P.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 62; NO 1-2; PP. 245-247; BIBL. 10 REF.Article
THE EXCITATION OF THE OXYGEN METASTABLE OI(1S) STATE IN METEORS.BAGGALEV WJ.1976; BULL. ASTR. INST. CZECHOSL.; CZECHOSL.; DA. 1976; VOL. 27; NO 3; PP. 173-181; ABS. RUSSE; BIBL. 40 REF.Article
OBSERVATION OF SUBORDINATE 2P54D-2P53P TRANSITIONS IN NEON-LIKE IONS FROM CAXI TO NIXIX.KASTNER SO; BEHRING WE; COHEN L et al.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 199; NO 3 PART. 1; PP. 777-780; BIBL. 7 REF.Article
EFFECTS OF A FREE-FREE RADIO CONTINUUM ON THE POPULATION OF HIGH ATOMIC LEVELS AT LOW TEMPERATURES AND DENSITIES.AHMAD IA.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 194; NO 2 PART. 1; PP. 503-512; BIBL. 25 REF.Article
RADIATIVE AND PREDISSOCIATION PROBABILITIES FOR INDIVIDUAL ROTATIONAL LEVELS OF THE B2SIGMA - STATE OF CH WITH APPLICATION TO THE RADIATIVE RECOMBINATION OF CH IN THE INTERSTELLAR MEDIUM.BROOKS NH; SMITH WH.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 194; NO 2 PART. 1; PP. 513-517; BIBL. 24 REF.Article
SEMIEMPIRICAL CALCULATION OF GF VALUES. III. INTERSTELLAR LINES OF THE IRON GROUP.KURUCZ RL.1974; SMITHSON. ASTROPHYS. OBS. SPEC. REP.; U.S.A.; DA. 1974; NO 360; PP. (62P.); ABS. FR. RUSSE; BIBL. 2 P.Article