Our objective in this study is to resolve phylogeny and taxonomic uncertainties for
Gyps taxa, in order to inform current conservation efforts. By using museum specimens as DNA sources along with tissues obtained from the field, we sampled representatives of all generally recognized
Gyps taxa with emphasis on those geographically distributed in south Asia; the primary area experiencing recent, drastic population declines. Our analyses support two changes to the traditional taxonomy for
Gyps. First, two individuals identified as
G. f. fulvescens were most closely related to
G. himalayensis (Figs. , ). Relatively high divergence estimates among all
G. fulvus individuals (1.5–2.5%, Table
1) and relatively low divergence estimates between
G. f. fulvescens and
G. himalayensis (0.0–0.6%) reflect this phylogenetic result. Additional sampling and analyses for
G. f. fulvescens are needed to verify these results. Second, our analyses based on both morphological and molecular data indicate the phylogenetic distinctiveness of the Long-billed and the Slender-billed Vultures, supporting their taxonomic treatment as distinct species (e.g.,
G. indicus and
G. tenuirostris, respectively) as recommended previously [
29-
31]. Mensural analyses show that
indicus and
tenuirostris differ significantly in proportions, especially of the head, wing, and pes (Table
2), and all individuals in each taxon are clearly separated on at least one axis in a PCA (Table
3). In our molecular analyses, pairwise sequence divergences between
G. indicus and
G. tenuirostris are similar to their respective divergence estimates from
G. coprotheres (Table
1), and to those reported between various other broadly recognized species within the family Accipitridae [
35]. These results highlight the utility of molecular phylogenetic methods in identifying independent evolutionary lineages within a group that has a long history of taxonomic uncertainty [
3,
27,
28,
32-
35,
37-
39], and, furthermore, help identify and resolve problematic specimen identifications (i.e.,
fulvescens; see also [
17,
40]).
The phylogenetic relationships found among
Gyps vultures were largely the same for the different methods and mt datasets. Despite our finding of monophyly for the majority of
Gyps species, relatively small sequence difference estimates (0.5–3.8%; Table
1) separating some named species made determination of sister relationships difficult, and multiple relationships were unresolved due to low nodal support. This suggests that the
Gyps study taxa stem from relatively rapid and recent diversification events. If we use a generally supported avian mtDNA divergence rate for coding regions ranging from 1.6 to 5.0% change per million years (see [
41]), our mt cytB and ND2 sequence divergence estimates (GTR+G; 0.8–3.4%), indicate that the radiation of
Gyps vulture study species occurred 0.2 to 2.1 million years ago. These estimates must be considered with caution as they assume clock-like rates of sequence change, which is known to be violated in comparisons of some avian taxa and genes (e.g. [
42-
45]). However, we were not able to reject a hypothesis of clock-like behavior for our particular
Gyps sequence dataset using a log likelihood ratio test (-ln L
clock = 3743.13, -ln L
non-clock = 3731.94; 2Δln L = 22.38; d.f. = 18; P > 0.05). Even if we assume that the above divergence rates are too high (see [
45]), a lower rate (e.g., 0.6% per million years) still yields divergence times that are quite recent (< 5.7 million years).
These divergence estimates do not necessarily correspond with geographic proximity or the current distributions of species. For example, divergence estimates between
G. indicus and both
G. coprotheres and
G. rueppellii are relatively low (0.9–1.3%; cytB & ND2 combined), yet the species compared occupy different continents. In contrast, divergence estimates between species with geographically proximate distributions,
G. coprotheres and
G. africanus in Africa and
G. i. tenuirostris and
G. himalayensis in South Asia (see Fig. ) are relatively high (2.9–3.2% and 2.8–3.1%, respectively).
The historic radiation of this genus likely evolved in environmental conditions that no longer exist to the same extent throughout their current distributions.
Gyps species are unique among Old World vultures in that they feed exclusively as scavengers, whereas other vultures are also known to kill their prey on occasion or, rarely, to feed on fruits (i.e.,
Gypohierax angolensis; [
2,
3,
21]. This specialization in feeding behavior among
Gyps vultures is thought to have evolved due to their close association with ungulate populations, particularly migratory populations in Africa and Asia. In fact, the observed temporal and geographic diversification of
Gyps vultures coincides with the diversification of Old World ungulates, especially in the family Bovidae [
46-
50], and the expansion of grass-dominated ecosystems in Africa and Asia (see [
51]). These close associations likely played a significant role in the adaptation and rapid diversification of
Gyps vultures. Indeed, Houston [
2] proposed that their large body size and ability to soar over large distances in search for food are related to the associated migrant distributions and seasonal fluctuations in mortality of ungulates, and that they have consequently become incapable of actually killing their own prey (see also [
52]).