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J/A+A/367/597       ups Her, phi Her & HR 7018 abundances     (Adelman+, 2001)

Elemental abundance analyses with DAO spectrograms. XXIV. The Mercury Manganese stars υ Her, φ Her, and HR 7018 Adelman S.J., Gulliver A.F., Rayle K.E. <Astron. Astrophys. 367, 597 (2001)> =2001A&A...367..597A
ADC_Keywords: Stars, peculiar ; Abundances, peculiar ; Equivalent widths Keywords: stars: abundances - stars: individual: υ Her - stars: individual: φ Her - stars: individual: HR 7018 - stars: chemically peculiar Abstract: Elemental abundances analyses are performed for the Mercury-Manganese stars υ Her, φ Her, and HR 7018 consistent with previous studies of this series using spectrograms obtained with Reticon and CCD detectors. Comparisons of the first two analyses with those performed using coadded photographic plates show the general consistency of the derived elemental abundances. For υ Her and for φ Her, abundances were newly found for O, and for Al, V, Zn, and Ce, respectively. HR 7018 is discovered to be a single-lined spectroscopic binary. Its Sc abundance is the smallest of any class member with derived abundances and its Sr abundance the largest of any known HgMn star. A correlation analysis of the most complete abundance sets for 20 HgMn stars shows that the abundances of some elements are correlated with one another and some are functions of the stellar effective temperature. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 16 02 47.9 +46 02 12 upsilon Her = 6 Her = HD 144206 16 08 46.2 +44 56 06 phi Her = 11 Her = HD 145389 18 37 33.5 +62 31 36 HR 7018 = HD 172728 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table6a.dat 69 627 Elemental abundances table6b.dat 43 33 Relative abundances table6.tex 101 973 LaTeX version of table 6
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/MNRAS/316/514 : 28 And + 99 Her elemental abundances (Adelman+, 2000) 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: table6a.dat
Bytes Format Units Label Explanations
1- 6 A6 --- Ion Ion designation 8- 10 A3 --- Mult Multiplet number from Moore (1945) if first line of multiplet, if not from Moore an initial indicating the paper (1) 12- 19 F8.2 0.1nm lambda Laboratory wavelength (air) 21- 25 F5.2 --- loggf Oscillator strength 28- 29 A2 --- r_loggf Reference to oscillator strength (2) 31- 33 I3 0.1pm EW1 ? Equivalent width for υ Her 35- 39 F5.2 --- log(N/Ntot)1 ? Relative abundance value for υ Her 41- 43 I3 0.1pm EW2 ? Equivalent width for φ Her 45- 49 F5.2 --- log(N/Ntot)2 ? Relative abundance value for φ Her 51- 53 I3 0.1pm EW3 ? Equivalent width for HR 7018 55- 58 F4.2 --- log(N/Ntot)3 ? Relative abundance value for HR 7018
Note (1): The acronyms are: D: Dworestsky, 1971, Ph.D. Thesis, University of California, Los Angeles G: Guthrie, 1985MNRAS.216....1G H: Huldt et al., 1982, Phys. Scripta 25, 401 I: Iglesias & Velasco, 1964, Publ. Inst. Opt. Madrid, No. 23 J: Johansson, 1978, Phys. Scr., 18, 217 K: Kurucz & Bell 1995, Kurucz CD-Rom No. 23 S: Svendenius et al., 1983, Phys. Scr. 27, 339 Note (2): gf value references follow: BG = Biemont et al. (1989A&A...209..391B) for V II; Biemont et al. (1981ApJ...248..867B) for Zr II BK = Biemont et al. (1982A&A...107..166B) GB = Grevesse et al. (1981, Upper Main Sequence CP Stars, 23rd. Liege Astrophys. Coll., 211) 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) JK = Joensson et al. (1984, Phys. Rev. A, 30, 2429) JS = Jugaku et al. (1961ApJ...134..783J) 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, Cat. VI/72) & Martin, Fuhr & Wiese (1988, Cat. VI/72) MC = Magazzu & Cowley (1986ApJ...308..254M) VA = from Vienna Atomic Line Database 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 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)
Byte-by-byte Description of file: table6b.dat
Bytes Format Units Label Explanations
1- 6 A6 --- Ion Ion 8- 10 A3 --- El Element 12- 16 F5.2 --- log(El/Ntot)1 ? Elemental abundance for upsilon Her (1) 18- 21 F4.2 --- e_log(El/Ntot)1 ? rms uncertainty on log(El/Ntot)1 23- 27 F5.2 --- log(El/Ntot)2 ? Elemental abundance for phi Her (1) 29- 32 F4.2 --- e_log(El/Ntot)2 ? rms uncertainty on log(El/Ntot)2 34- 38 F5.2 --- log(El/Ntot)3 ? Elemental abundance for HR 7018 (1) 40- 43 F4.2 --- e_log(El/Ntot)3 ? rms uncertainty on log(El/Ntot)3
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 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 Ryabchokova 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
(End) Patricia Bauer CDS 15-Jan-2001
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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