Type of variability: DCEP

These are the classical cepheids, or Delta Cep-type variables. Com- paratively young objects that have left the main sequence and evolved into the instability strip of the Hertzsprung-Russell (H-R) diagram, they obey the well-known Cepheid period-luminosity relation and belong to the young disk population. DCEP stars are present in open clusters. They display a certain relation between the shapes of their light curves and their periods.

General Catalog of Variable Stars

529

stars

0

observed in last month


Name Type Brightness
T ANT DCEP 8.88 – 9.8
ETA AQL DCEP 3.48 – 4.3
FM AQL DCEP 7.89 – 8.6
KL AQL DCEP 9.82 – 10.5
PP AQL DCEP 11.6 – 13.4
SZ AQL DCEP 7.92 – 9.2
TT AQL DCEP 6.46 – 7.7
U AQL DCEP 6.08 – 6.8
V0336 AQL DCEP 9.5 – 10.2
V0493 AQL DCEP 10.79 – 11.3
V0600 AQL DCEP 9.73 – 10.4
V0733 AQL DCEP 9.73 – 10.1
V0912 AQL DCEP 12.5 – 13.7
V0916 AQL DCEP 11.6 – 13.2
V0979 AQL DCEP 14.1 – 14.8
V1183 AQL DCEP 14.4 – 15.7
V1307 AQL DCEP 17.1 – 18.1
V1344 AQL DCEP 7.65 – 8.0
V1495 AQL DCEP 14.0 – 15.0
V1496 AQL DCEP 12.5 – 13.4