Fig. 3 from Time Series Spectroscopy of Pulsating Subdwarf B Stars: PG 1605+072

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Time Series Spectroscopy of Pulsating Subdwarf B Stars: PG 1605+072

Authors: S. J. O'Toole, T. R. Bedding, H. Kjeldsen, T. C. Teixeira, G. Roberts, F. van Wyk, D. Kilkenny, N. D'Cruz, and I. K. Baldry

O'Toole et al. 2000 The Astrophysical Journal Letters 537 L53.

Provider: AAS Journals

Caption: Fig. 3.

Velocity amplitude vs. wavelength for the five Balmer lines studied. The group of unresolved modes at 2.10 mHz is represented by diamonds, while the mode at 2.74 mHz is represented by triangles.

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