ERRATUM: âEXPLORING B4: A PULSATING sdB STAR ... - IOPscience
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ERRATUM: âEXPLORING B4: A PULSATING sdB STAR ... - IOPscience
Apr 17, 2012 - doi:10.1088/2041-8205/750/1/L26. C 2012. ... The x-axis in Figure 1 of the original paper was incorrectly scaled. The range of the figure should ...
The Astrophysical Journal Letters, 750:L26 (1pp), 2012 May 1 C 2012.
doi:10.1088/2041-8205/750/1/L26
The American Astronomical Society. All rights reserved. Printed in the U.S.A.
ERRATUM: “EXPLORING B4: A PULSATING sdB STAR, IN A BINARY, IN THE OPEN CLUSTER NGC 6791” (2011, ApJ, 740, L47) Herbert Pablo1 , Steven D. Kawaler1 , and Elizabeth M. Green2
2
1 Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA Received 2012 March 23; published 2012 April 17
The x-axis in Figure 1 of the original paper was incorrectly scaled. The range of the figure should go from 0 to 1.6 days. The correct Figure 1 is printed here. We have also changed the axis label and figure caption for clarity. 0.02 0.015
Differential Flux
0.01 0.005 0 -0.005 -0.01 -0.015
0
0.2
0.4
0.6
1 0.8 Phase(Days)
1.2
1.4
Figure 1. Photometric data on B4, phased on twice the suspected orbital period (2 × 0.3885 days). The equal-depth minima argue against an interpretation of the light curve as being caused by ellipsoidal variation.
