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J/MNRAS/520/6111
-1
Spectrophotometric magnetic study of MWD stars (Hardy+, 2023)
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2023MNRAS.520.6111H
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1.
J/MNRAS/520/6111/table6
Atmospheric and dipole geometry parameters for hydrogen-rich MWD stars but are moderately well modelled with a dipolar geometry
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(45 rows)
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J/MNRAS/520/6111/table6
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Constraint
Explain
(
UCD
)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
meta.record
)
(
RECORD
)
Name
(char)
Object name designation as JHHMM±DDMM based on ICRS coordinates at Ep=J2000 and Eq=J2000 (J_Name)
(
meta.id;meta.main
)
(
ID_MAIN
)
Teff
K
Effective temperature derived from spectral fits analysis (T
eff
)
(
phys.temperature.effective
)
(
PHYS_TEMP_EFFEC
)
e_Teff
K
Uncertainty of Teff
(
stat.error;phys.temperature.effective
)
(
ERROR
)
logg
[cm/s2]
Logarithm of the surface gravity derived from spectral fits analysis (logg)
(
phys.gravity
)
(
PHYS_GRAVITY_SURFACE
)
e_logg
[cm/s2]
Uncertainty of logg
(
stat.error
)
(
ERROR
)
M*
Msun
Stellar mass derived from spectral fits analysis (Mass)
(
phys.mass
)
(
PHYS_MASS_MISC
)
e_M*
Msun
Uncertainty of M*
(
stat.error
)
(
ERROR
)
Bp
10-7T
The dipole intensity B
p
as magnetic field intensity at the pole of a centred dipole at the stellar surface (1R
*
from the otigin) (B
p
)
(
phys.magField
)
(
PHYS_MAG-FIELD
)
i
deg
The inclination angle i between the dipole moment m ant the observer's line of sight (i)
(Note 1)
(
src.orbital.inclination
)
(
POS_INCLIN_LOS
)
az/R*
The distance between the centre of the dipole and the centre of the star in units of stellar radius R* (a
z
)
(
pos.distance
)
(
PHYS_DISTANCE_TRUE
)
Bmean
10-7T
Mean of dipole magnetic field intensity on the visible surface of the star
(
phys.magField;stat.mean
)
(
PHYS_MAG-FIELD
)
sp
Display the spectrum fit results for stars moderately well modelled with a dipolar geometry
(
meta.ref.url
)
(
DATA_LINK
)
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