Fig. 1 from On the Origin of Long Secondary Periods in Semiregular Variables

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT 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. 1.

Spectra for two variables Z Eri (M‐type) and U Hya (C‐type). The spectrum of Z Eri clearly shows the TiO band heads, which are characteristic of M star spectra. Note that these spectra are not corrected for heliocentric motion.

Other Images in This Article

Copyright and Terms & Conditions