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J/AJ/149/59
594
Abundances of ρ Pup (Yushchenko+, 2015)
ReadMe+ftp
2015AJ....149...59Y
Similar Catalogs
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1.
J/AJ/149/59/table1
Iron lines in the spectrum of ρ Pup
(167 rows)
meta
J/AJ/149/59/table1
2.
J/AJ/149/59/table2
Abundances of chemical elements in the atmosphere of ρ Pup: individual lines
(430 rows)
meta
J/AJ/149/59/table2
3.
J/AJ/149/59/table3
Abundances of chemical elements in the atmosphere of ρ Pup: mean values
(73 rows)
meta
J/AJ/149/59/table3
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Column
Constraint
Explain
(
UCD
)
(ALL)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
meta.record
)
(
RECORD
)
(1+2)
M
(char)
M
ean abundance for this element
(
meta.ref.url
)
(
DATA_LINK
)
(ALL)
Ion
(char)
Iron line identifier (Fe I or Fe II)
(
phys.atmol.ionStage
)
(
AT_ION_ID
)
(1+2)
lambda
0.1nm
[4620/8839] Wavelength λ; in Å
(
em.wl
)
(
SPECT_WAVELENGTH_MISC
)
(1+2)
loggf
[-]
[-5.24/0.53] Log of the oscillator strength
(
phys.atmol.oscStrength
)
(
AT_OSC_STRENGTH
)
(1+2)
r_loggf
Reference for loggf
(Note G2)
(
meta.ref;phys.atmol
)
(
REFER_CODE
)
(1+2)
Elow
eV
[0/10.48] Lower level energy
(
phys.energy;phys.atmol.level
)
(
AT_ENERGY_LEVEL
)
(1)
EW
0.1pm
[4/198] Equivalent width; in mÅ
(
spect.line.eqWidth
)
(
SPECT_EQ-WIDTH
)
(1)
logN
[-]
[7.783/8.03] Log number abundance
(Note G3)
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(2+3)
Tel
(char)
Telescope facility used (IUE or VLT)
(Note G1)
(
meta;instr.setup
)
(
TEL_ID
)
(2)
logN*
[-]
Log number absolute abundance in ρ Pup
(Note G3)
(
phys.abund
)
(
PHYS_ABUND_MISC
)
ALL
cols
(i)
indexed column
(2)
logNo
[Sun]
(n)
Log number absolute abundance in the Sun
(Note G3)
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(2)
Abund
[Sun]
Difference between logN* and logNS
(Note 1)
(
phys.abund;arith.diff
)
(
PHYS_ABUND_MISC
)
(2)
Inp*
Relative input of the investigated line to the line absorption coefficient in synthetic spectrum of ρ Pup (1=Clean line, 0=Very weak line)
(Note 2)
(
meta.note
)
(
SPECT_FEATURE_PROP
)
(2)
Inpo
(n)
Relative input of the investigated line to the line absorption coefficient in synthetic spectrum of the Sun (1=Clean line, 0=Very weak line)
(Note 2)
(
meta.note
)
(
SPECT_FEATURE_PROP
)
(2)
Depth*
Depth of line in synthetic spectrum of ρ Pup
(
phys.absorption.opticalDepth
)
(
SPECT_LINE_DEPTH_VALUE
)
(2)
Deptho
(n)
Depth of line in synthetic spectrum of the Sun
(
phys.absorption.opticalDepth
)
(
SPECT_LINE_DEPTH_VALUE
)
(2)
d(T)
[-]
(n)
Change in logN* for T
eff
=+100K
(Note 3)
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(2)
d(g)
[-]
(n)
Change in logN* for logg=-0.3
(Note 3)
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(3)
Z
[3/90] Atomic number
(
meta.id;meta.main
)
(
AT_NUMBER
)
(3)
Nl
[1/120] Number of lines used
(
phys.abund
)
(
NUMBER
)
(3)
Abest
[Sun]
Best value mean abundance (ρ Pup minus Solar)
(Note 1)
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(3)
e_Abest
[Sun]
(n)
1σ uncertainty in Abest
(
stat.error
)
(
ERROR
)
(3)
A+100K
[Sun]
Mean abundance (ρ Pup minus Solar) with effective temperature increased by +100K
(
phys.abund
)
(
PHYS_ABUND_MISC
)
ALL
cols
(n)
indicates a possible blank or NULL column
(i)
indexed column
(3)
e_A+100K
[Sun]
(n)
1σ uncertainty in A+100K
(
stat.error
)
(
ERROR
)
(3)
Ag+0.2
[Sun]
Mean abundance (ρ Pup minus Solar) with surface gravity decreased by +0.2cm/s
2
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(3)
e_Ag+0.2
[Sun]
(n)
1σ uncertainty in Ag+0.2
(
stat.error
)
(
ERROR
)
(3)
Nbest
[-]
Best value of ρ Pup absolute mean abundance
(Note 2)
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(3)
e_Nbest
[-]
(n)
1σ uncertainty in Nbest
(
stat.error
)
(
ERROR
)
(3)
N+100K
[-]
Absolute mean abundance of ρ Pup with effective temperature increased by +100K
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(3)
e_N+100K
[-]
(n)
1σ uncertainty in N+100K
(
stat.error
)
(
ERROR
)
(3)
Ng+0.2
[-]
Absolute mean abundance of ρ Pup with surface gravity decreased by +0.2cm/s
2
(
phys.abund
)
(
PHYS_ABUND_MISC
)
(3)
e_Ng+0.2
[-]
(n)
1σ uncertainty in Ng+0.2
(
stat.error
)
(
ERROR
)
ALL
cols
(n)
indicates a possible blank or NULL column
(i)
indexed column
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