The agglomeration of small clusters of the coinage metals in noble gas
matrices to form larger ones may be accompanied by the emission of li
ght in the spectral range 280-1000 nm. Spectral analysis reveals that
the part of the radiation intensity can be attributed to fluorescence
of excited metal species Me-n (n = 1, 2, 3). A mechanism is proposed,
according to which the gain in binding energy upon cluster formation m
ay even lead to the ejection of excited fragments via unstable interme
diate configurations. The other so far unknown emission bands were par
tly attributed to larger clusters (n greater than or equal to 4). This
assignment was confirmed by the discovery of the respective so far un
known absorption bands of extremely low oscillator strength.