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J/MNRAS/316/514 28 And & 99 Her elemental abundances (Adelman+, 2000)
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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 (SIMBAD/NED BibCode)
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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:
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RA (2000) DE Designation(s) (Sp)
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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)
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table4a.dat 54 1262 Elemental abundances
table4b.dat 34 38 Relative abundances
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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)
Byte-by-byte Description of file: table4a.dat
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Bytes FormatUnits Label Explanations
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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)
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Note (1): 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, ApJS, 94, 22
Note (2): Sources of gf-values:
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)
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: Jonsson et al. (1984, Phys. Rev. A, 30, 2429)
KX: Kurucz (1995, ASP Conf. Ser. 78, 205)
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)
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)
Note (3): N = number of atoms/volume of particular element
Ntot = number of atoms/volume of all elements
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Byte-by-byte Description of file: table4b.dat
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Bytes Format Units Label Explanations
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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
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Note (1): El = Element
Ntot = number of atoms/volume of all elements
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Acknowledgements: Saul J. Adelman <ADELMANS@adelvx.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
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
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(End) Patricia Bauer [CDS] 17-Feb-2000