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Recently, extra motivation has been given to the investigations of anunresolved problem of millisecond pulsars (MSPs) produced by the recyclingprocess, as an apparent role of the accretion-induced collapse (AIC) in whitedwarfs (WDs) was suggested to this concern. I have found that the distributionof the orbital periods of binary MSPs in the Galactic disk closely follows anexponential distribution. I have also determined the best-fit mean value ofNobs by fitting our data with an exponential distribution for the MSPpopulation. As a result, it can be stated that reaching the Chandrasekhar limitmay cause an explosion of a massive WD as a Type Ia supernova (in the case of aCO WD) or an ignition of a ONeMg WD, and possibly merging in some CO WDs, allresulting in peculiar MSP systems. A possible formation scenario, where thesystem has a circular orbit during this evolutionary stage, is discussed.

Accretion-Induced Collapse of White Dwarfs as an Alternative Symbiotic Channel to Millisecond Pulsars