We present and discuss the second list of the Montreal Blue Galaxy sur
vey. Following the inspection of 71 plates, we found 237 new candidate
s with B<15.5. 73 percent of them are also detected by IRAS. Spectroph
otometry was carried out, at medium resolution, for a subset of 40 obj
ects leading to the identification of three new AGNs and producing 13
new radial velocities. Spectral. classification of our candidates conf
irms our previous finding that the majority of our candidates are star
burst nucleus galaxies similar to the objects studied by Balzano [ApJ,
268, 602 (1983)]. Our survey is biased against the high excitation st
arburst H II galaxies and the LINER galaxies. Metallicities of our gal
axies are found to be from log (O/H)=8.4 to 9.0, which suggests galaxi
es in advanced stages of chemical evolution.