Narrow band photometry of Wolf-Rayet stars
Abstract
In this thesis results are presented from a study of
intermediate dispersion spectra, and six-colour narrow hand
photometry of Wolf-Rayet (WR) stars in the southern Milky Way and in
the Magellanic Clouds.
Until very recently photometric data on WR stars have been
appallingly lacking. Westerlund and Smith (196*0 have obtained
photographic B,V, R colours for most of the WR stars in the Large
Magellanic Cloud (IMC), and Feast, Thackeray, and Wesselink (i960)
have obtained U, B,V colours for a few. However, in the Galaxy, U,B,V
colours have been obtained for only about one-third of the known WR
stars (Demers and Femie, 1964; Feinstein, 1964; Hiltner, Schild
and Jackson, 1964; Hiltner and Iriarte, 1955; Hiltner, 1956;
Cousins and Stoy, 196 3).
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