Abstract
| In Chapter 6 the difficulties in using Strömgren photometry for Be
star analysis were highlighted and an attempt was made to separate
the constituent parts, (E(b - y)cs, E(b - y)is and (b - y)0). The
method produced results which were well correlated, but the results also
contained large errors. Chapter 7 devised a new method of separating the
observed flux from a Be star which provided highly correlated results
with low errors, this chapter will use this technique on the representative
sample of Strömgren photometry previously presented and analysed in
Chapter 6. It is hoped that this approach will develop smaller errors and
hence produce more reliable results. |
The greatest pleasure in life is doing what people say you cannot do.
Walter Bagehot
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