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Sinterizazio-atmosferaren eragina M graduko (ASP 30 ... - Euskara

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in Table V the carbonitrides are richer in Vanadium than than the corresponding<br />

carbides. This has also been observed in other high speed steels sintered in<br />

nitrogen atmospheres (17,18) . It is worth emphasising that the MX carbonitrides in<br />

gas sintered specimens present a mean particle size smaller than 1 um, while MC<br />

carbides after vacuum sintering have mean sizes between 3 and 4 µ m, except for<br />

Px<strong>30</strong>S +0.2%C with a mean size of around 2 pm . The presence of these fine<br />

carbonitrides, rich in vanadium, has been reported by other authors both after direct<br />

sintering in a nitrogen rich atmosphere (17,18) and after nitrogenation and hipping<br />

(27) . The presence of these carbonitrides, which are not dissolved at high<br />

temperatures, can explain the features observed in Figs 5a and 5b . In these figures<br />

is shown the austenite grain size evolution as a function of the deviation from<br />

optimum sintering temperature . For both steels, with a substantial amount of MX<br />

carbonitrides for atmosphere sintering (see Table IV), oversintering has only a minor<br />

effect in grain growth, while in vacuum sintering oversintering produces fast<br />

austenite grain size growth . No appreciable effect has been found for carbon<br />

addition. Using the expression of Zener (28) for the relation between the limiting<br />

grain size (d) and the size (r) and volume fraction (f) of second phase dispersion :<br />

d = 4r/3f<br />

and using the data of Table IV refering to volume fraction and size of dispersed<br />

particles the values, summarized in Table VIII _for the limiting grain size at_ the__<br />

optimum sintering temperature are obtained . As shown in the table, in which also the<br />

experimental values are given, the values proposed by the Zener equation are<br />

around a half the values experimentally observed for Px<strong>30</strong> steel ; the same proportion<br />

is also observed for Px<strong>30</strong>S steel gas sintered, but the experimental values are<br />

around three times bigger than those proposed by the Zener expression for vacuum<br />

sintering . The important increment in the grain size taking place in vacuum sintering<br />

(Fig . 5) is essentially due to a decrease in the volume fraction of M 6C carbides with<br />

oversintering . These effect has also been reported for a T42 steel (17) . The finer<br />

particles and the maintenance of the volume fraction of the carbonitrides with<br />

oversintering in the atmosphere sintered specimens explain the small increase in<br />

grain size with oversintering (see Fig . 5) .

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