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| Paper: |
Analysis of the B and Be Star Populations of the Double Cluster h and χ Persei |
| Volume: |
465, Four Decades of Massive Star Research - A Scientific Meeting in Honor of Anthony J. Moffat |
| Page: |
422 |
| Authors: |
Marsh Boyer, A. N.; McSwain, M. V. |
| Abstract: |
We present blue optical spectra of 92 members of h and χ Per obtained with the WIYN 3.5m telescope. From the spectra, several stellar parameters were measured for the B-type stars, including V sin i, Teff, log gpolar, M★, and R★. Strömgren photometry was used to measure Teff and log gpolar for the Be stars. Additional photometry is used to examine the spectral energy distributions of the Be stars, giving some preliminary insight into the disk structures present. |
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