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VizieR

The 4 columns in color are computed by VizieR, and are not part of the original data.
J/ApJ/837/96/table4 Rotation-Activity Correlations in K-M dwarfs II. (Houdebine+, 2017)
Equivalent width of the Ca II resonance doublet and Hα line for our sample of dM3 stars (see Houdebine & Mullan, 2015ApJ...801..106H) (83 rows)
img(gal)
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Full

Star

N

l_

CaH-H
0.1nm
e_
(...)
l_

CaK-H
0.1nm
e_
(...)
Ha-H
0.1nm
e_
(...)
CaH-S
0.1nm
e_
(...)
CaK-S
0.1nm
e_
(...)
Ha-S
0.1nm
e_
(...)
K/H

l_

<Ca>
0.1nm
f_

All

SimbadName

_RA
deg
_DE
deg
1Gl 752A13,7   -0.784 0.01   -0.910 0.01 0.338 0.020 -0.72 0.02 -1.16 0.02 0.375 0.020 1.16   -0.828  AllGl 752A289.23024+05.16890
J/ApJ/837/96/table5 Rotation-Activity Correlations in K-M dwarfs II. (Houdebine+, 2017)
The values of vsin(i), P/sin(i) and [M/H] from Paper I (Houdebine+ 2016, J/ApJ/822/97) for our targets in our list of dM3 stars (97 rows)
img(gal)
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Full

Star

l_

vsini
km/s
l_

Per
d
e_
d
E_
d
[M/H]
[Sun]
CaII
0.1nm
FHK
10+4mW/m2
FHKc
10+4mW/m2
All

SimbadName

_RA
deg
_DE
deg
1Gl 752A   1.19  21.20 4.30 6.70 0.045 -0.828 2.549 2.298AllGl 752A289.23024+05.16890
J/ApJ/837/96/table8 Rotation-Activity Correlations in K-M dwarfs II. (Houdebine+, 2017)
The log(LHK), log(Lbol), R'HK and R0 for our samples of dK4, dK6, dM2, dM3 and dM4 stars (384 rows)
img(gal)
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SpT

Star

logLHK
[10-7W]
logLHKc
[10-7W]
logLbol
[10-7W]
R'HK

R'HKc

logLX
[10-7W]
logLX/Lb
[-]
R0

f_

HCat

All

SimbadName

_RA
deg
_DE
deg
1M3Gl 752A26.89026.84532.122-5.233-5.278     0.17440   0AllGl 752A289.23024+05.16890
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