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CONSERVATION OF ARABIAN GAZELLES - Nwrc.gov.sa

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Table 2.7 Skeletal postcranial measurements for cenain Arabian gazelles<br />

(data from both sexes combined).<br />

Humerus Foreleg: Tibia: Metatar<strong>sa</strong>l: Hindleg:<br />

length hindleg femur femur skull<br />

gazella (20) 125 78 127 100 302<br />

dorcas ( II) 119 81 133 III 314<br />

<strong>sa</strong>udiya (I) 116 80 130 109 298<br />

sub8utturo<strong>sa</strong> (10) 125 81 127 109 290<br />

Discussion<br />

It is probable that, according to a Phylogenetic Species Concept, all the following taxa would be<br />

regarded as separate species: <strong>sa</strong>udiya, arabica, bilkis, erlangeri, gazella, muscatensis, and cora. The<br />

status of marica vis-a-vis C. subgutturo<strong>sa</strong> was not tested, but both morphologically (Groves &<br />

Harrison, 1967) and genetically (Kingswood et al., this volume) there is ample reason to regard it as<br />

pan of the <strong>sa</strong>me species. Similarly, there seems little doubt that i<strong>sa</strong>bella and other forms of G.<br />

dorcas are con specific (Groves, 198Ib). As little other than metrical data was collected on the<br />

Thumarnah crania, the position of this quasi-taxon on the cladogram remains somewhat hypothetical.<br />

The status of the other taxa will be discussed in tum.<br />

- Status of Gazellil <strong>sa</strong>udiya: That Cazella <strong>sa</strong>udiya is totally distinct from C. dorcas is<br />

confirmed; as Rebholz et al. (this volume) have concluded, it is much closer to C. bennetti. It would<br />

be difficult to propose uniting them specifically, however. Metrically, C. <strong>sa</strong>udiya falls outside the<br />

range of variation of C. bennetti, and the skull is a different shape from the similarly small-sized C. b.<br />

karamii (Table 2.4). In addition it shares some derived states with C. subgutturo<strong>sa</strong> which are not<br />

seen in C. bennetti (Figure 2.6): na<strong>sa</strong>l tip shortening, ethmoid fissure shape, greater sexual size<br />

difference, horn length in both sexes, more hom rings. Unless the polarities of these characters are<br />

incorrect, or there is an unsuspected degree of homoplasy, this does imply that C. bennetti and G.<br />

<strong>sa</strong>udiya may not be sister species.<br />

A question that must be asked is whether the AI-Areen (Bahrain) breeding group,<br />

phenetically resembling C. <strong>sa</strong>udiya, is pure-bred or has been mixed with C. bennetti (see Rebholz et<br />

al., this volume, for discussion). The only detailed evidence is the morphology (mainly craniometry)<br />

of a female specimen made available courtesy of Dr Jaime Samour, formerly of the AI-Areen<br />

Wildlife Park . This specimen (Table 2.4) is considerably larger than wild-collected C. <strong>sa</strong>udiya in the<br />

Natural History Museum, London (the only existing study <strong>sa</strong>mple), but is in proportion; compared to<br />

C. bennetti, it has a narrow skull, especially the braincase and across the hom bases, and the na<strong>sa</strong>ls<br />

are narrower posteriorly than anteriorly. The horns are extremely long, like C. <strong>sa</strong>udiya, and spread<br />

more widely than either (on average), though they would be easily within the 2-standard-deviation<br />

limits of C. <strong>sa</strong>udiya; but it must be borne in mind that the female of C. bennetti karamii, whose horns<br />

are exceptionally widely flared for that species, is unknown . In Figure 2.5 this skull, entered as an<br />

unknown in a Discriminant Analysis comparing C. bennetti and C. <strong>sa</strong>udiya, falls within the range of<br />

the latter, confirming its identity in shape.<br />

There is consequently only one character in which the AI-Areen specimen falls outside the<br />

expected range of C. <strong>sa</strong>udiya: absolute size. It is possible that this is an effect of captivity (see the<br />

discussion above on subspecies and phenotypic plasticity); it is also possible that it derives from a<br />

population outside the known area of distribution of C. <strong>sa</strong>udiya (Appendix 2. I).<br />

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