Published August 31, 2021
| Version v1
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Fig. 1 in Interactive identification key to all brittle star families (Echinodermata; Ophiuroidea) leads to revised morphological descriptions
Authors/Creators
- 1. Ferdowsi University of Mashhad, Faculty of Science, Department of Biology, Mashhad, Iran. & Ghent University, Research Group Evolutionary Morphology of Vertebrates, Gent, Belgium. & Mona.
- 2. Swedish Museum of Natural History, Department of Zoology, Stockholm, Sweden.
- 3. Ferdowsi University of Mashhad, Faculty of Science, Department of Biology, Mashhad, Iran. & Research Department of Zoological Innovations (RDZI), Institute of Applied Zoology, Faculty of Science, Ferdowsi University of Mashhad, Mashhad, Iran.
- 4. Ferdowsi University of Mashhad, Faculty of Science, Department of Biology, Mashhad, Iran
- 5. Ghent University, Research Group Evolutionary Morphology of Vertebrates, Gent, Belgium. & Dominique.
Description
Fig. 1. Dorsal disc shapes and radial shields in brittle stars as defined for the purpose of this study. A. Flat (Ophioderma sp.). B. High, with bar-like radial shields (Asteronyx loveni Müller & Troschel, 1842 (dry specimen)). C. Sac-like, radial shields absent (Ophiotholia spathifer (Lyman, 1879)). D. Thick skin obscuring scales and plates (Ophiosparte gigas Koehler, 1922). E. Flat, radial shield scalene triangular to half circle (Amphiura chiajei Forbes, 1843). F. Arm combs, radial shields isosceles triangular to pearshaped (Ophiura ophiura (Linnaeus, 1758)).
Notes
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