“…They are: H2-He, H2 (Michaut et al 1998), 12 CH 3 D-He, H 2 , N 2 (Boussin et al 1999), H 2 S-He, H 2 , N 2 , 0 2 (Flatin et al 1999), CO-He, Ar (Sinclair et al 1998), C0 2 -He, Ar, C 0 2 , N 2 , 0 2 (Rodrigues et al 1998, Vigasin 1999, Ma et al 1999, De Rosa et al 1999, N 2 -N 2 (Buldyreva et al 1999), NH 3 -H2,NH 3 (Irwin et al 1999, Birnbaum et al 2000, N 2 0 -He, N 2 , l e 0 2 -1 6 0 2 (Schermaul k Learner 1999), 1 Collision Induced Spectra Collision-induced absorption in dense atmospheres of cool stars has been reviewed by Borysow and Jorgensen (1999). Recent publications include studies of far-infrared bands of H 2 , C0 2 , O2 and liquid methane (Brodbeck et al 1999, Gruszka k Borysow 1999, Moreau et al 2000, Birnbaum et al 1999, and of the fundamental band of CO broadened by N 2 (Luo et al 1999).…”