The paper ‘The variable star population in the globular cluster NGC 6934’ was published in RMxAA, 54, 15 (2018). Several identifications of variable stars in the chart of figure 9 are erroneous. The stars involved are V7 and V8, V94 and V95. The correct identifications of these stars are now shown in the present chart in Figure 1. For completeness we have now identified the candidate variable stars C2, C3, C4 and C5. The candidate C1 is out of the field of these charts. The equatorial coordinates of C2 and C3 in the original table 2 are interchanged. In present Table 1 the correct coordinates are given. The rest of the entries of table 2 of the original paper are correct.
Variable Star ID |
Variable Type |
<
V > (mag) |
<
I > (mag) |
AV (mag) |
AI (mag) |
P (KOS01) (d) |
HJDmax (+ 2 450 000) |
P (this work) (d) |
RA (J2000.0) |
Dec (J2000.0) |
---|---|---|---|---|---|---|---|---|---|---|
C2a | SX Phe | 19.96 | 19.51 | 0.09 | 0.18 | - | 5780.4479 | 0.006961 | 20:34:10.1 | 07:24:55 |
C3a | SX Phe | 19.968 | 19.6 | 0.18 | 0.15 | - | 5779.4293 | 0.061280 | 20:34:13.3 | 07:23:32 |