  Cyg X-1 was observed in the high state at the conjunction orbital phase (0)
with HETG/Chandra. Strong and asymmetric absorption lines of highly ionized
species were detected, such as Fe XXV, Fe XXIV, Fe XXIII, Si XIV, S XVI, Ne X,
and etc. In the high state the profile of the absorption lines are composed of
an extended red wing and a less extended blue wing. The red wings of higher
ionized species are more extended than that of lower ionized species. The
detection of these lines provides a way to probe the properties of the flow
around the companion and the black hole in Cyg X-1 during the high state. A
broad emission feature around 6.5 keV was significantly detected from the both
spectra of HETG/Chandra and PCA/RXTE. This feature appears to be symmetric and
can be fitted with a Gaussian function rather than the Laor disk line model of
fluorescent Fe K$_\alpha$ line from an accretion disk. The implications of
these results on the structure of the accretion flow of Cyg X-1 in the high
state are discussed.
