The star formation history of Trumpler 14 and Trumpler 16

H-R diagrams are presented for the very young galactic clusters Trumpler 14 and Trumpler 16, which are the two most populous clusters in the region of vigorous star formation surrounding eta Carinae. Point spread function pho tometry of UBV CCD images is presented down to V approximate to 19 for over 560 stars in Tr 16 and 290 stars in Tr 14. We have also obtained similar d ata for a local background field. After determining cluster membership thro ugh proper motions from a previous work, we find that the reddening of clus ter members is significantly lower than that of the local background stars. Thus, we are able to use individual reddenings to identify likely members at far deeper levels than possible with proper motions. This work has revea led a significant population of pre-main-sequence (PMS) stars in both clust ers. The location of the PMS stars in the H-R diagram indicates that the th eoretical "stellar birthline" of Palla & Stahler follows the locus of stars far better than that of Beech & Mitalas. Comparison with both pre- and pos t-main-sequence isochrones also reveals that although intermediate-mass sta rs have been forming continuously over the last 10 Myr, the high-mass stars formed within the last 3 Myr. There is no evidence that the formation of t he intermediate-mass stars was truncated by the formation of the high-mass stars.