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J/A+A/447/685       Elemental abundance analyses. XXIX.      (Adelman+, 2006)

Elemental abundance analyses with DAO spectrograms XXIX. The Mercury-Manganese stars 53 Tau, beta Tau, gamma Crv, and upsilon Her. Adelman S.J., Caliskan H., Gulliver A.F., Teker A. <Astron. Astrophys. 447, 685 (2006)> =2006A&A...447..685A
ADC_Keywords: Stars, peculiar ; Abundances, peculiar Keywords: stars: abundances - stars: chemical peculiar - stars: individual: 53 Tau, beta Tau, gamma Crv, upsilon Her Abstract: We performed elemental abundances analyses of the mercury-manganese (HgMn) stars 53 Tau, β Tau, and γ Crv consistent with previous studies of similar stars in this series. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 04 19 26.1 +21 08 32 53 Tau = V* V1024 Tau 05 26 17.5 +28 36 27 beta Tau = * 112 Tau 12 15 48.4 -17 32 31 gamma Crv = * 4 Crv 16 02 47.9 +46 02 12 ups Her = * 6 Her ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 20 26 He/H determinations tab567.dat 54 667 Abundances for β Tau, γ Crv, 53 Tau and from newly measured lines of υ Her abund.dat 32 73 Atomic abundances table8.dat 32 56 Comparison of Results (logN/H) for 53 Tau, γ Crv, and υ Her last analysis with this paper tables.tex 91 856 LaTeX version of the tables
See also: J/A+A/354/899 : Elemental abundance analyses IV. (Adelman+, 2000) J/A+A/367/597 : ups Her, phi Her + HR 7018 (XXIV) (Adelman+, 2001) J/A+A/367/859 : α Scl and HD 170973 abundances (Lopez-Garcia+, 2001) J/A+A/371/1078 : Elemental abundance analyses XXV (Adelman+, 2001) J/A+A/394/187 : γ Ser + 101 Her (XXVI) (Caliskan+, 2002) J/A+A/406/975 : Elemental abundance analyses XXVII (Kocer+, 2003) J/A+A/406/987 : Elemental abundances of three CP stars (Pintado+, 2003) J/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994) J/A+AS/125/219 : mu Lep, 7 Sex, HR 4817 + 28 Her (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 (II)_ (Lopez-Garcia+ 1999) J/MNRAS/316/514 : 28 And + 99 Her (XXIII) (Adelman+, 2000) Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star name 12- 15 I4 0.1nm lambda Wavelength 17- 20 F4.2 --- He/H He/H abundace value (1)
Note (1): Average values: 53 Tau : He/H = 0.042±0.008 beta Tau : He/H = 0.070±0.010 gamma Crv : He/H = 0.067±0.010
Byte-by-byte Description of file: tab567.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star name 11- 16 A6 --- Ion Ion 19- 23 A5 --- Mult Multiplet number (1) 25- 31 F7.2 0.1nm lambda Laboratory wavelength 34- 38 F5.2 --- log(gf) log gf value 41- 42 A2 --- r_log(gf) Reference for log(gf) (2) 45- 47 I3 0.1pm EWlambda ?=- Equivalent width 50- 54 F5.2 --- log(Nel/Ntot) ?=- Derived abundance
Note (1): Multiplet number from Moore 1945 if first line of multiplet; if not from Moore an initial indicating the paper Note (2): gf value references are as follows: BG = Biemont et al. (1981ApJ...248..867B) GB = Grevesse et al. (1981, Upper Main Sequence CP Stars, 23rd. Liege Astrophys. Coll., 211) DW = Dworetsky (1980A&A....84..350D) 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) KX = Kurucz & Bell (1995, Kurucz CD-Rom No. 23) LA = Lanz & Artru (1985PhyS...32..115L) LD = Lawler & Dakin (1989, JOSA B, 6, 1457) MF = Fuhr, Martin & Wiese, 1988, and Martin, Fuhr & Wiese, 1988, Cat. VI/72 N4 = Fuhr & Wiese (2005, "A Critical Compilation of Atomic Transition Probabilities for Neutral and Singly-Ionized Iron", J. Phys. Chem. Ref. Data, in press) SG = Schulz-Gulde (1969, JQSRT, 9, 13) WF = Wiese, Fuhr & Deters (1996, Atomic transition probabilities of carbon, nitrogen, and oxygen : a critical data compilation. Edited by W.L. Wiese, J.R. Fuhr, and T.M. Deters. Washington, DC) WM = Wiese & Martin (1980, NSRDS-NBS 68. Part 2, US Government Printing Office, Washington, DC) WS = Wiese, Smith & Glennon (1966, NSRDS-NBS 4, US Governement Printing Office, Washington) and Wiese, Smith & Miles (1969, NSRDS-NBS, D.C.: US Department of Commerce, National Bureau of Standards)
Byte-by-byte Description of file: abund.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star name 11- 16 A6 --- Ion Ion 19- 20 A2 --- Element Element (identical to bytes 11-12) 23- 27 F5.2 --- log(Nel/Ntot) Derived abundance of element (1) 29- 32 F4.2 --- e_log(Nel/Ntot) ? rms uncertainty on (Nel/Ntot)
Note (1): Ratio of number of atoms to the total number of atoms per unit volume
Byte-by-byte Description of file: table8.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star name 12- 17 A6 --- Ion Ion 21- 25 F5.2 --- log(Nel/H)old Previous relative abundance (1) 28- 32 F5.2 --- log(Nel/H) This Paper relative abundance
Note (1): Previous log(Nel/H) values are from Paper II (Adelman, 1987MNRAS.228..573A) for 53 Tau, Fremat & Houziaux ( 1997A&A...320..580F) for γ Crv, Paper XXIV (Adelman et al., 2001, Cat. J/A+A/367/597 for υ Her
Acknowledgements: Saul J. Adelman, adelmans(at)citadel.edu References: Moore, 1945, A multiplet table of astrophysical interest, Princeton, N.J., The Observatory, 1945. Rev. ed. Adelman & Hill, Paper I 1987MNRAS.226..581A Adelman, Paper II 1987MNRAS.228..573A Adelman, Paper III 1988MNRAS.230..671A Adelman, Paper IV 1988MNRAS.235..749A Adelman, Paper V 1988MNRAS.235..763A Adelman, Paper VI 1989MNRAS.239..487A Adelman, Paper VII 1991MNRAS.252..116A Adelman et al., Paper VIII 1991MNRAS.252..329A Bolcal et al., Paper IX 1992MNRAS.258..270B Adelman, Paper X 1992MNRAS.258..167A Pintado & Adelman, Paper XI 1993MNRAS.264...63P Adelman, Paper XII 1994MNRAS.266...97A Adelman, Paper XIII 1994MNRAS.271..355A Ryabchikova et al., Paper XIV 1996MNRAS.283.1115R Adelman, Paper XV 1996MNRAS.280..130A Adelman et al., Paper XVI 1997MNRAS.288..470A Caliskan & Adelman, Paper XVII 1997MNRAS.288..501C Adelman et al., Paper XVIII 1998MNRAS.297....1A Adelman, Paper XIX 1998MNRAS.296..856A Adelman & Albayrak Paper XX 1998MNRAS.300..359A Adelman et al. Paper XXI 1999MNRAS.305..591A Adelman Paper XXII 1999MNRAS.310..146A Adelman et al. Paper XXIII 2000MNRAS.316..514A, Cat. J/MNRAS/316/514 Adelman et al. Paper XXIV 2001A&A...367..597A, Cat. J/A+A/367/597 Adelman et al. Paper XXV 2001A&A...371.1078A, Cat. J/A+A/371/1078 Caliskan et al. Paper XXVI 2002A&A...394..187C, Cat. J/A+A/394/187 Kocer et al. Paper XXVII 2003A&A...406..975K, Cat. J/A+A/406/975
(End) Patricia Vannier [CDS] 07-Oct-2005
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

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