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J/MNRAS/515/1903
-1
Stars cluster and RGBs study in NGC362 (Vargas+, 2022)
ReadMe+ftp
2022MNRAS.515.1903V
Similar Catalogs
Post annotation
1.
J/MNRAS/515/1903/table2
Atmospheric parameters for the 11 target stars derived with isochrone fits
(11 rows)
meta
J/MNRAS/515/1903/table2
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Constraint
Explain
(
UCD
)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
meta.record
)
(
RECORD
)
ID
Star identifier number (ID)
(
meta.id;meta.main
)
(
ID_MAIN
)
TeffGaiam11
K
Effective temperature obtained via 11 Gyr isochrone fitting using Gaia data (T
GAIAm11
)
(
phys.temperature.effective;meta.modelled
)
(
PHYS_TEMP_EFFEC
)
loggGaiam11
[cm/s2]
Logarithm of the surface gravity obtained via 11 Gyr isochrone fitting using Gaia data (g
GAIAm11
)
(
phys.gravity;meta.modelled
)
(
PHYS_GRAVITY_SURFACE
)
TeffGaiam09
K
Effective temperature obtained via 9 Gyr isochrone fitting using Gaia data (T
GAIAm09
)
(
phys.temperature.effective;meta.modelled
)
(
PHYS_TEMP_EFFEC
)
loggGaiam09
[cm/s2]
Logarithm of the surface gravity obtained via 9 Gyr isochrone fitting using Gaia data (g
GAIAm09
)
(
phys.gravity;meta.modelled
)
(
PHYS_GRAVITY_SURFACE
)
TeffHSTm11
K
Effective temperature obtained via 11 Gyr isochrone fitting using HST data (T
HSTm11
)
(
phys.temperature.effective;meta.modelled
)
(
PHYS_TEMP_EFFEC
)
loggHSTm11
[cm/s2]
Logarithm of the surface gravity obtained via 11 Gyr isochrone fitting using HST data (g
HSTm11
)
(
phys.gravity;meta.modelled
)
(
PHYS_GRAVITY_SURFACE
)
TeffHSTm09
K
Effective temperature obtained via 9 Gyr isochrone fitting using HST data (T
HSTm09
)
(
phys.temperature.effective;meta.modelled
)
(
PHYS_TEMP_EFFEC
)
loggHSTm09
[cm/s2]
Logarithm of the surface gravity obtained via 9 Gyr isochrone fitting using HST data (g
HSTm09
)
(
phys.gravity;meta.modelled
)
(
PHYS_GRAVITY_SURFACE
)
loggphot
[cm/s2]
Logarithm of the surface gravity obtained with the canonical relation as the described in section 4 (logg
phot
)
(
phys.gravity;meta.modelled
)
(
PHYS_GRAVITY_SURFACE
)
Teff
K
Effective temperature used to compute v
t
and [Fe/H] (Teff)
(
phys.temperature.effective;meta.modelled
)
(
PHYS_TEMP_EFFEC
)
logg
[cm/s2]
Logarithm of the surface gravity used to compute v
t
and [Fe/H] (logg)
(
phys.gravity;meta.modelled
)
(
PHYS_GRAVITY_SURFACE
)
Vt
km/s
Microturbulent velocity obtained assuming T
eff
, log(g) and FeI line spectra (vt)
(
phys.veloc.microTurb;meta.modelled
)
(
VELOC_MICRO-TURB
)
[Fe/H]
[Sun]
Iron to hydrogen abundance ratio assuming T
eff
, log(g) and FeI line spectra ([Fe/H])
(
phys.abund.Fe;arith.ratio;meta.modelled
)
(
PHYS_ABUND_FE/H
)
[FeII/H]
[Sun]
Derived ionic iron FeII to hydrogen abundance ratio ([FeII/H])
(
phys.abund.Fe;arith.ratio;meta.modelled
)
(
PHYS_ABUND_FE/H
)
Class
(char)
[a/n] Star classification a for anomalous and n for normal (Class)
(
src.class
)
(
CLASS_MISC
)
ALL
cols
(i)
indexed column
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https://cdsannotations.u-strasbg.fr/annotations/vizierTable//
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