Figure 3.
The MV–〈V〉 relations for the different formulae connecting the absolute magnitudes of RRab stars with their light-curve parameters. Solid lines in all panels have a slope of unity. Filled circles correspond to MV values computed from our formulae and open circles to the formulae of KW01. The MV values obtained from KW01 equations are shifted by 0.4 mag for clarity.

The MV–〈V〉 relations for the different formulae connecting the absolute magnitudes of RRab stars with their light-curve parameters. Solid lines in all panels have a slope of unity. Filled circles correspond to MV values computed from our formulae and open circles to the formulae of KW01. The MV values obtained from KW01 equations are shifted by 0.4 mag for clarity.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close