  Supersoft X-ray (SSX) fluxes in early type galaxies provide an excellent test
for type Ia supernova (SN Ia) progenitors: Double degenerate (DD) scenario is
believed to produce no SSXs except just before SN Ia explosion, while single
degenerate (SD) scenario produces in some phase of the symbiotic channel.
Recent observations of SSX flux of early type galaxies show a remarkable
agreement with theoretical prediction of SD scenario, which is thus turn to be
a strong support for SD scenario, despite the original observation aimed at the
opposite conclusion. Here I explain why X-ray fluxes are so weak in early type
of galaxies: (1) Candidate binaries in SD scenario become supersoft X-ray
source only in a short time on its way to an SN Ia explosion, because it spend
a large part of lifetime as wind phase, (2) During the supersoft X-ray phase,
symbiotic stars emit very weak SSX fluxes even if the WD is very massive. It
should be emphasized that SSX symbiotic stars are very rare and we need more
observation to understand their nature.
