Image Details

Choose export citation format:

On the Origin of Long Secondary Periods in Semiregular Variables

  • Authors: E. A. Olivier and P. R. Wood

Olivier & Wood 2003 The Astrophysical Journal 584 1035.

  • Provider: AAS Journals

Caption: Fig. 2.

Power spectra of the flux spectra of U Hya and V Hya plotted against the square of the frequency. The top and bottom panels are for orders 80 (7030–7160 Å) and 84 (6700– 6800 Å), respectively. Left panels: unbroadened spectra of U Hya. Right panels: rotationally broadened spectra of U Hya with the noise of the original power spectrum added. Power spectra are normalized at 0.5 cycles Å−1.

Other Images in This Article
Copyright and Terms & Conditions