Fig. 11 from A Photometric and Spectroscopic Study of the Cataclysmic Variable ST LMi during 2005

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

A Photometric and Spectroscopic Study of the Cataclysmic Variable ST LMi during 2005–2006

Authors: S. Kafka, S. B. Howell, R. K. Honeycutt, and J. W. Robertson

Kafka et al. 2007 The Astronomical Journal 133 1645.

Provider: AAS Journals

Caption: Fig. 11.

Line profiles of He I λ5876 (left column), Hα (middle column), and He I λ6678 (right column) as a function of orbital phase, for the high‐state spectra of 2006 May 19 UT. The NaD emission lines (from Tucson airglow) are often visible near and sometimes within the red wing of He I λ5876.

Other Images in This Article

Copyright and Terms & Conditions