J/MNRAS/316/514     28 And & 99 Her elemental abundances     (Adelman+, 2000)

Elemental abundance analyses with DAO spectrograms. XXIII. The superficially normal stars 28 And (A7 III) and 99 Her (F7 V). Adelman S.J., Caliskan H., Kocer D., Hamami I., Tektunali H.G. <Mon. Not. R. Astron. Soc. 316, 514 (2000)> =2000MNRAS.316..514A 2000MNRAS.316..514A
ADC_Keywords: Stars, normal ; Abundances, peculiar ; Equivalent widths Keywords: abundances - stars: individual: 28 And - stars: individual: 99 Her - delta Scuti Abstract: Elemental abundances of 28 And (A7III) and 99 Her (F7V), which have modest rotational velocities, are derived in a manner consistent with previous studies in this series of papers. The values for 28 And, a δ Scuti variable, show that it is slightly metal-poor, but not a classical Am star. 99 Her, which is somewhat more metal-poor, has a rather small microturbulence for its spectral type. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) (Sp) ---------------------------------------------------------- 00 30 07.4 +29 45 06 28 And = HR 114 (A7 III) 18 07 01.5 +30 33 44 99 Her = HR 6775 (F7 V) ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4a.dat 54 1262 Elemental abundances table4b.dat 34 38 Relative abundances -------------------------------------------------------------------------------- See also: J/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994) J/A+AS/125/219 : mu Lep, 7 Sex, HR 4817 & 28 Her abundances (Adelman+ 1997) J/A+AS/129/563 : Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998) J/A+AS/137/227 : HD 133029 & HD 192913 abundances (Lopez-Garcia+ 1999) J/A+A/367/597 : ups Her, phi Her & HR 7018 abundances (Adelman+, 2001) J/A+A/367/859 : α Scl and HD 170973 abundances (Lopez-Garcia+, 2001) J/A+A/371/1078 : alpha Dra, tau Her, gamma Lyr, HR 7926 (Adelman+, 2001) J/A+A/394/187 : γ Ser & 101 Her elemental abundances (Caliskan+, 2002) J/A+A/406/975 : theta And, eps Del, eps Aqr, iota And (Kocer+, 2003) J/A+A/406/987 : xi Oct, alpha Sex, 68 Tau elemental abund. (Pintado+, 2003) Byte-by-byte Description of file: table4a.dat -------------------------------------------------------------------------------- Bytes FormatUnits Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Ion Ion 7- 11 A5 --- No Multiplet number from Moore (1945) if first line of multiplet, if not from Moore an initial indicating the paper (1) 13- 19 F7.2 0.1nm Lambda Laboratory wavelength (air) 22- 26 F5.2 --- log(gf) Oscillator strength 29- 30 A2 --- r_log(gf) Reference to oscillator strength (2) 33- 35 I3 0.1pm EW1 ? Equivalent width for 28 And 37- 42 F6.2 --- log(N/Ntot)1 ? Elemental abundance for 28 And (3) 45- 47 I3 0.1pm EW2 ? Equivalent width for 99 Her 49- 54 F6.2 --- log(N/Ntot)2 ? Elemental abundance for 99 Her (3) -------------------------------------------------------------------------------- Note (1): the acronyms are: C: Catalan et al., 1964, J. Res. NBS, 68A, 9 J: Johansson S., 1978, Phys. Scripta, 18, 217 K: Kurucz & Bell 1995, Kurucz CD-Rom No. 23 MCS: Meggers et al., 1975, Tables of Spectral-Line Intensities, US Goverment Printing Office, Washington, DC N: Nave et al., 1994, Cat. J/ApJS/94/221 Note (2): Sources of gf-values: BG: Biemont et al. (1989A&A...209..391B 1989A&A...209..391B) for V II; Biemont et al. (1981ApJ...248..867B 1981ApJ...248..867B) for Zr II BK: Biemont et al. (1982A&A...107..166B 1982A&A...107..166B) FW: Fuhr & Wiese (1990, in Lide D.R. ed., CRC Handbook of Chemistry and Physics, CRC Press, Cleveland, OH) HL: Hannaford et al. (1982ApJ...261..736H 1982ApJ...261..736H) JK: Jonsson et al. (1984, Phys. Rev. A, 30, 2429) KX: Kurucz (1995, ASP Conf. Ser. 78, 205) LA: Lanz & Artru (1985PhyS...32..115L 1985PhyS...32..115L) LD: Lawler & Dakin (1989, JOSA B, 6, 1457) MF: Fuhr, Martin & Wiese (1988, Cat. VI/72) & Martin, Fuhr & Wiese (1988, Cat. VI/72) MC: Magazzu & Cowley (1986ApJ...308..254M 1986ApJ...308..254M) MW: Miles & Wiese (1969, NBS Technical Note No. 474) YF: Younger et al. (1978, J. Phys. Chem. Ref. Data, 7, 495) WF: Wiese, Fuhr & Deters (1996, J. Phys. Chem. Ref. Data, Monograph 6) WM: Wiese & Martin (1980, NSRDS-NBS 68, Part.2, US Governement Printing Office, Washington) WS Wiese, Smith & Glennon (1966, NSRDS-NBS 4, US Governement Printing Office, Washington) & Wiese, Smith & Miles (1969, NSRDS-NBS, D.C.: US Department of Commerce, National Bureau of Standards) WV Ward (1985MNRAS.213...71W 1985MNRAS.213...71W) Note (3): the designations are: N = number of atoms/volume of particular element Ntot = number of atoms/volume of all elements -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4b.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Ion Ion 8- 9 A2 --- El Element 11- 16 F6.2 --- log(El/Ntot)1 ? Elemental abundance for 28 And (1) 18- 21 F4.2 --- e_log(El/Ntot)1 ? rms uncertainty on log(El/Ntot)1 23- 28 F6.2 --- log(El/Ntot)2 ? Elemental abundance for 99 Her (1) 30- 33 F4.2 --- e_log(El/Ntot)2 ? rms uncertainty on log(El/Ntot)2 -------------------------------------------------------------------------------- Note (1): El = Element Ntot = number of atoms/volume of all elements -------------------------------------------------------------------------------- Acknowledgements: Saul J. Adelman References: Moore, 1945, A multiplet table of astrophysical interest, Princeton, N.J., The Observatory, 1945. Rev. ed. Adelman & Hill, Paper I 1987MNRAS.226..581A 1987MNRAS.226..581A Adelman, Paper II 1987MNRAS.228..573A 1987MNRAS.228..573A Adelman, Paper III 1988MNRAS.230..671A 1988MNRAS.230..671A Adelman, Paper IV 1988MNRAS.235..749A 1988MNRAS.235..749A Adelman, Paper V 1988MNRAS.235..763A 1988MNRAS.235..763A Adelman, Paper VI 1989MNRAS.239..487A 1989MNRAS.239..487A Adelman, Paper VII 1991MNRAS.252..116A 1991MNRAS.252..116A Adelman et al., Paper VIII 1991MNRAS.252..329A 1991MNRAS.252..329A Bolcal et al., Paper IX 1992MNRAS.258..270B 1992MNRAS.258..270B Adelman, Paper X 1992MNRAS.258..167A 1992MNRAS.258..167A Pintado & Adelman, Paper XI 1993MNRAS.264...63P 1993MNRAS.264...63P Adelman, Paper XII 1994MNRAS.266...97A 1994MNRAS.266...97A Adelman, Paper XIII 1994MNRAS.271..355A 1994MNRAS.271..355A Ryabchokova et al., Paper XIV 1996MNRAS.283.1115R 1996MNRAS.283.1115R Adelman, Paper XV 1996MNRAS.280..130A 1996MNRAS.280..130A Adelman et al., Paper XVI 1997MNRAS.288..470A 1997MNRAS.288..470A Caliskan & Adelman, Paper XVII 1997MNRAS.288..501C 1997MNRAS.288..501C Adelman et al., Paper XVIII 1998MNRAS.297....1A 1998MNRAS.297....1A Adelman, Paper XIX 1998MNRAS.296..856A 1998MNRAS.296..856A Adelman & Albayrak, Paper XX 1998MNRAS.300..359A 1998MNRAS.300..359A Adelman et al., Paper XXI 1999MNRAS.305..591A 1999MNRAS.305..591A Adelman, Paper XXII 1999MNRAS.310..146A 1999MNRAS.310..146A
(End) Patricia Bauer [CDS] 17-Feb-2000
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line