  Supernovae descendent from massive stars explode in media that have been
modified by their progenitors' mass loss and UV radiation. The supernova ejecta
will first interact with the circumstellar material shed by the progenitors at
late evolutionary stages, and then interact with the interstellar material.
Circumstellar nebulae in supernova remnants can be diagnosed by their small
expansion velocities and high [N II]/H$\alpha$ ratios. The presence of
circumstellar nebulae appears ubiquitous among known young supernova remnants.
These nebulae can be compared to those around evolved massive stars to assess
the nature of their supernova progenitors. Three types of archeological
artifacts of supernova progenitors have been observed in supernovae and/or
young supernova remnants: (1) deathbed ejecta, (2) circumstellar nebulae, and
(3) interstellar bubbles. Examples of these three types are given.
