We report high-resolution angle resolved photoemission studies of 2H-NbSe2
and 2H-TaS2. Results are compared to those of 2H-TaSe2. We find that the no
rmal stare electronic structures in this family of materials have the same
basic characteristics. Their Fermi surface consists of a pocket around Gamm
a and another one around K. They ail exhibit a saddle band near EF along T-
K. A finite energy gap is observed in the saddle band region and on the Fer
mi surface around K in 2H-TaS2 and 2H-TaSe2. Gapping on the Fermi surface a
round Gamma was not observed. We suggest that the charge density waves in t
his family of materials originate from a combination of the partial nesting
of the Fermi surface around K and the saddle band.