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Journal of Paleontology 92(3):432–441
not fused between each other around the opesia-orifice, but connected in the marginal and proximal zones of the zooid. Opesia-orifice wider than long, 120 µm long × 260 µm wide, its proximal margin bent upward as a lappet consisting of three acute projections that may be lost during preservation. At both sides of the proximal margin there is an indistinct lateral notch with a small projection sinking in distobasal direction. Vicarious avicularia longer than the autozooids, 751 × 322 µm, located at the bifurcation of zooid rows. The acute rostrum covers one of the proximal corners of the distal zooid, the boundary V-shaped. Avicularian cryptocyst with small isolated granules and a pair of subequal, large reniform opesial foramina. Rostral foramen subelliptical, with a medioproximal projection. Lateral and distal walls with rounded, multiporous pore plates. Ovicells not observed.
Etymology.—From Latin bi, meaning two or double, and perforare, to bore; referring to the paired opesial foramina of the avicularium.
Other material.—Two fragments, MPEF-PI 6350, Punta del Marqués, Chubut Province. Chenque Formation.
Remarks.—We assigned this new species to Melychocella mainly due to the presence of vicarious avicularia with rostral and opesial foramina. It differs from M. cynura Gordon and Taylor, 1999, the type species of this genus, by lacking the pair of distal condyles in the opesia-orifice. M. biperforata n. sp. differs from the other species of the genus by having a pair of reniform opesial foramina in the avicularia.
Discussion
Aspidostoma giganteum can be easily distinguished from the new fossil species described in this study by the greater size of the autozooids. At around 1170 × 820 µm, the zooids are considerably larger than in most species of cheilostome bryozoans. Its gigantism might be related to its present distribution in cold-temperate waters of the Magellanic Region. However, several cheilostome species, mainly distributed in
Antarctica and in subpolar seas (Grischenko et al., 2002), are known with zooids that exceed the size of A. giganteum. Aspidostoma incrustans can also be set clearly apart from
other fossil species of Aspidostoma by the presence of huge pores piercing its cryptocyst.Onthe other hand, A. ortmanni, A. armatum, A. tehuelche,and A. roveretoi exhibit a common morphological pattern. Each is characteristic of a particular geological unit (Fig. 6) and can be distinguished by the morphological features summarized in Table 1. Aspidostoma ortmanni is characterized by having very small avicularia, A. armatum by its concave quadrangular process and its relatively large avicularia, A. tehuelche by its protruding avicularia and its avicularian cystides in contact with two auto- zooids, and A. roveretoi by its regularly hexagonal or rhombic zooids with strongly depressed central cryptocysts (Table 1). The fact that Melychocella biperforata was found by us in both
the Monte León and the Chenque formations, and that M. flammula and Aspidostoma incrustans were originally described by Canu (1908) from the Punta Borja (Chenque Formation) and were found during the present study in the Monte León Formation (Fig. 6), suggests that the upper levels of the Monte León Formation might correlate with the lower levels of the Chenque Formation. In addition to the species treated in this study, the Aspidos-
tomatidae of the southern tip of South America are represented by four Paleogene taxa: A. onychocelliferumCanu, 1911, A. globifera Canu, 1911 (Roca Formation, early Paleocene, Río Negro Pro- vince), A. hexagonalis Canu, 1904, and A. porifera Canu, 1904 (San Julián Formation, late Oligocene, Santa Cruz Province). Three species of Melychocella were already known fromthe
Paleogene of the Chatham Islands, New Zealand (Southwest Pacific):M. cynura Gordon and Taylor, 1999, M. obliqua Gordon and Taylor, 2015, and M. bilamellata Gordon and Taylor, 2015. No representatives of this genus had been recorded yet outside the Chatham Islands. The occurrence of two species of Melychocella in the Neogene of Patagonia expands the temporal range of the genus and lends further support to the hypothesis of a close link between the faunas of the southern tip of South America and the Australasian region during the early Miocene, as has been dis- cussed in detail in previous studies (Casadío et al., 2010; Pérez et al., 2015; López-Gappa et al., 2017).
Figure 6. Chronostratigraphic chart showing the age of the formations analyzed in this study and their species. The solid line within each rectangle indicates the approximate level of the bryozoan fossil associations. *Species recorded by Canu (1908) for Punta Borja, Chenque Formation.
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