VizieR Search Page
[
Back
] ⋅ [
Forwd
] ⋅ [
Print
] ⋅ [
Close
]
JavaScript is used, and should be enabled to get full functionality.
VI/109
756
Population Synthesis Models at very low metallicities (Schaerer, 2003)
ReadMe+ftp
2003A&A...397..527S
Similar Catalogs
Post annotation
1.
VI/109/type20
Main output (file corresponding to output described in Schaerer & Vacca,
1998ApJ...497..618S
) plus additional quantities (last four columns)
(74289 rows)
meta
VI/109/type20
Simple Constraint
List Of Constraints
Query by
Constraints
applied on Columns
(
Output Order:
+
-
)
Show
Sort
Column
Constraint
Explain
(
UCD
)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
meta.record
)
(
RECORD
)
Z
(char)
Code for metallicity Z
(Note G1)
(
phys.abund.Z
)
(
PHYS_ABUND_Z
)
mup
solMass
Upper mass cut-off of IMF in M
☉
(Note G1)
(
stat.param
)
(
MODEL_PARAM
)
low
solMass
Lower mass cut-off of IMF in M
☉
(Note G1)
(
stat.param
)
(
MODEL_PARAM
)
sfh
(char)
Code for star formation history (G1) (cs1, cs3, cs4, is1, is3)
(
stat.param
)
(
MODEL_PARAM
)
log(Age)
[yr]
Age
(
time.age
)
(
TIME_AGE
)
Mbol
mag
Bolometric magnitude
(
phys.magAbs.bol
)
(
PHOT_ABS-MAG_BOL
)
log(Q0)
[s-1]
Lyman continuum photon flux (Q
0
=Q
H
)
(
phot.flux.density;spect.continuum
)
(
SPECT_FLUX_UV
)
log(Q1)
[s-1]
He0 ionising photon flux (Q
1
=Q
He
)
(
phot.flux
)
(
SPECT_FLUX_UV
)
log(Q2)
[s-1]
He+ ionising photon flux (Q
0
=Q
He+
)
(
phot.flux
)
(
SPECT_FLUX_UV
)
NOstar
Number of O stars
(
meta.number
)
(
NUMBER
)
ALL
cols
(i)
indexed column
WR/(WR+O)
Ratio of WR to WR+O stars
(
stat.param
)
(
MODEL_POP-SYNTHESIS
)
WR/O
Ratio of WR to O stars
(
stat.param
)
(
MODEL_POP-SYNTHESIS
)
WNL/(WR+O)
Ratio of WNL (late WN) to WR+O stars
(
stat.param
)
(
MODEL_POP-SYNTHESIS
)
WNE/(WR+O)
Ratio of WNE (early WN) to WR+O stars
(
stat.param
)
(
MODEL_POP-SYNTHESIS
)
WC/(WR+O)
Ratio of WC to WR+O stars
(
stat.param
)
(
MODEL_POP-SYNTHESIS
)
EWHb
0.1nm
Nebular Hβ equivalent width
(Note G2)
(
spect.line.eqWidth;em.line.Hbeta
)
(
SPECT_EQ-WIDTH
)
LHb
10-7W
Nebular Hβ luminosity
(Note G2)
(
phys.luminosity;em.line.Hbeta
)
(
PHYS_LUMINOSITY_HBETA
)
EWHeI
0.1nm
Nebular HeI 4471 equivalent width (CAUTION: Saturation effect !)
(Note G2)
(
spect.line.eqWidth
)
(
SPECT_EQ-WIDTH
)
LHeI
Relative Nebular HeI 4471 luminosity (in Hβ unit)
(Note G2)
(
phys.luminosity;em.line.Hbeta
)
(
PHYS_LUMINOSITY_HBETA
)
EWHeII
0.1nm
Nebular HeII 4686 equivalent width
(Note G2)
(
spect.line.eqWidth
)
(
SPECT_EQ-WIDTH
)
LHeII
Nebular HeII 4686 luminosity (in Hβ unit)
(Note G2)
(
phys.luminosity;em.line.Hbeta
)
(
PHYS_LUMINOSITY_HBETA
)
EWWR
0.1nm
WR bump (CIII/IV 4650 + HeII 4686) equivalent width
(
spect.line.eqWidth
)
(
SPECT_EQ-WIDTH
)
LWR
WR bump (CIII/IV 4650 + HeII 4686) luminosity (in Hβ unit)
(Note G2)
(
phys.luminosity;em.line.Hbeta
)
(
PHYS_LUMINOSITY_HBETA
)
EWCI
0.1nm
CI V-WR equivalent width
(
spect.line.eqWidth
)
(
SPECT_EQ-WIDTH
)
LCI
CI V-WR luminosity (in Hβ unit)
(Note G2)
(
phys.luminosity;em.line.Hbeta
)
(
PHYS_LUMINOSITY_HBETA
)
Balmer
mag
Balmer jump, defined as -2.5*log(F(3640Å)/F(3650Å)
(
phot.mag
)
(
SPECT_BALMER_JUMP
)
log(QH2)
[s-1]
Ionising photon flux in Lyman-Werner band (Q
H2
=Q
LW
)
(Note G3)
(
phot.flux
)
(
SPECT_FLUX_UV
)
E(Q)
eV
Average energy per photon in Lyman-continuum
(
stat.param
)
(
MODEL_ENERGY_DIST
)
E(QHe+)
eV
(n)
Average energy per photon with E>54eV
(
stat.param
)
(
MODEL_ENERGY_DIST
)
allQuantities
Display all output quantities for this model's parameters and age
(
meta.ref.url
)
(
DATA_LINK
)
ALL
cols
(n)
indicates a possible blank or NULL column
(i)
indexed column
Adapt form
Display your selection only
Reset to default columns
Display
UCD1+
UCD1
https://cdsannotations.u-strasbg.fr/annotations/vizierTable//
elapse time 1