Datatype: hk
This datatype (hk) collects the photoelectric photometric observations of
stars in open clusters made with the combination of Strögrem and
the Ca filters measuring the CaII HK line forming the Caby system.
The hk parameter is defined by : hk = (Ca - b) (b - y) by
Twarog et al. 1991.
CCD Caby observations are recorded under the hkccd datatype.
Record structure
No | : | Star number |
Ref | : | Reference |
V | : | V magnitude |
b-y | : | b-y colour index |
hk | : | hk parameter |
N | : | Number of measurements |
Database access
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Last Update: 16 April 2006