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Molecular Biology and Evolution, Vol 10, 1196-1214, Copyright © 1993 by Society for Molecular Biology and Evolution

ORIGINAL ARTICLE

Recovering phylogenetic signal from DNA sequences: relationships within the corvine assemblage (class aves) as inferred from complete sequences of the mitochondrial DNA cytochrome-b gene

K Helm-Bychowski and J Cracraft
Department of Chemistry, DePaul University.

Phylogenetic analysis of cytochrome-b sequences and cranial osteological characters for nine genera of corvine passerine birds supports the hypothesis that the two major groups of birds of paradise, the manucodines and paradisaeinines, constitute a monophyletic group and that their postulated sister group is the Corvidae (crows, jays, and allies). The data are also consistent with the hypothesis that the bowerbirds are not closely related to the birds of paradise but instead lie near the base of the corvine assemblage. The corvine radiation exemplifies a case of multiple star phylogenies embedded within a major clade, with the branching pattern characterized by very short internodal divergence times. Such histories are difficult to resolve no matter what type of data is employed, because little change accumulates between branching events. With respect to sequence data, reconstructed tree topologies are sensitive to the choice of outgroup and to the method of analysis (e.g., transversion vs. global parsimony). In such cases, assessing the "reliability" of a best-fit or most-parsimonious tree inferred from any particular data set becomes problematic. Statistical tests of tree topologies that depend on random sampling of characters will generally be inconclusive in that all cladistic components will tend to be poorly supported because relatively few character-state changes will be recorded between branching events. It is suggested, on the other hand, that congruence in cladistic signal across different data sets may be a potentially more useful method for evaluating the reliability of the signal of any one data set. Resolution of star phylogenies will probably be possible only if DNA sequence and morphological characters are combined in a single analysis.
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