plots: violin/box

Violin plots of 26Al/27Al in different chondrite types. Shown are ungrouped carbonaceous chondrites (C), High-metal-type (CH), Ivuna-type (CI), Murray-type (CM), Ornans-type (CO), Renazzo-type (CR), and Vigarano-type (CV) carbonaceous chondrites. H enstatite chondrites (EH) and H, L, and LL ordinary chondrites (OC). If there were two or less data points in one category, a violin plot was not drawn. The horizontal gray dashed line is the canonical 26Al/27Al ratio (5.23x10-5). 

Violin plots of 26Al/27Al in different CAI types. Shown are amoeboid olivine aggregates (AOA), type Bs, Type Cs, compact type A (CTA), fine-grained inclusion (FGI), fluffy-type A (FTA), and forsterite-olivine-bearing type B (FoB) which are primarily hosted in CV-type chondrites. Blue aggregates (BAG) and Spinel-hibonite-bearing (SHIB) inclusions are primarily from CM type meteorites. Anorthite-rich (an-rich), corundum grains (cor grains), grossite-rich (grs-rich), hibonite-corundum (hib-cor), hibonite-rich (hib-rich), melilite-rich (mel-rich), and spinel-rich (sp-rich) inclusions are defined based on their primary mineralogy and are from non-CV3 type meteorites. The isotopically anomalous CAIs additionally include fractionated-type (F), fractionated and unidentified nuclear (FUN), FUN inclusions with only hibonite, like HAL (FUN-hib), and platy hibonite crystal (PLACs). See paper for more information about these types. If there were two or less data points in one category, a violin plot was not drawn. The horizontal gray dashed line is the canonical 26Al/27Al ratio (5.23x10-5).