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Dolphinfish

Dolphinfish

UIG531671

Fishes: Perciformes Coryphaenidae (Dolphinfishes) Common dolphinfish (Coryphaena hippurus), illustration

Fishes: Perciformes Coryphaenidae (Dolphinfishes) Common dolphinfish (Coryphaena hippurus), illustration

DGA1140880

Fishes: Perciformes Stromateidae - Blue butterfish (Stromateus fiatola), illustration

Fishes: Perciformes Stromateidae - Blue butterfish (Stromateus fiatola), illustration

DGA1140892

Dolphinfish, 1833-39 (coloured engraving)

Dolphinfish, 1833-39 (coloured engraving)

French School, (19th century)

PRX999185

Beautiful fish (coloured engraving)

Beautiful fish (coloured engraving)

German School, (19th century)

PRX998318

Fishes: Perciformes Coryphaenidae - Common dolphinfish (Coryphaena hippurus), illustration

Fishes: Perciformes Coryphaenidae - Common dolphinfish (Coryphaena hippurus), illustration

DGA1141436

Marine Fishes: Remora, Dolphinfish, Tuna, Gurnard and Pike, 1821 (lithography)

Marine Fishes: Remora, Dolphinfish, Tuna, Gurnard and Pike, 1821 (lithography)

Bretzing, Georg (d.1876)

PRX11959553

10 cents coin, 1991, reverse, Common dolphinfish (Coryphaena hippurus), Malta, 20th century

10 cents coin, 1991, reverse, Common dolphinfish (Coryphaena hippurus), Malta, 20th century

DGA2588928

Coryphaena hippurus

Coryphaena hippurus

Forster, Georg (1754-94)

NHM1457519

Permit fish, Trachinotus falcatus, common dolphinfish or mahi mahi, Coryphaena pelagica, and sand tilefish, Malacanthus plumieri. Handcoloured copperplate engraving by Dequevauviller after an illustration by Jean-Gabriel Pretre from Bernard Germain de Lacepede's Natural History of Oviparous Quadrupeds, Snakes, Fish and Cetaceans, Eymery, Paris, 1825.

Permit fish, Trachinotus falcatus, common dolphinfish or mahi mahi, Coryphaena pelagica, and sand tilefish, Malacanthus plumieri. Handcoloured copperplate engraving by Dequevauviller after an illustration by Jean-Gabriel Pretre from Bernard Germain de Lacepede's Natural History of Oviparous Quadrupeds, Snakes, Fish and Cetaceans, Eymery, Paris, 1825.

FLO4655211

Dolphinfish, Coryphaena hippurus, pearly razorfish, Xyrichthys pendactylus, Atlantic pomfret, Brama raii, cuckoo wrasse, Labrus vetula, pearl-spot chromis, Chromis punctatus, palecheek parrotfish, Scarus viridis, banded archerfish, Toxotes jaculator, blotched picarel, Maena vulgaris, gilthead seabream, Sparus aurata, climbing perch, Anabas scandens, colisa, Polyacanthus colisa, and giant gourami. Lithograph from Lorenz Oken's Universal Natural History, Allgemeine Naturgeschichte fur alle Stande, Stuttgart, 1841.

Dolphinfish, Coryphaena hippurus, pearly razorfish, Xyrichthys pendactylus, Atlantic pomfret, Brama raii, cuckoo wrasse, Labrus vetula, pearl-spot chromis, Chromis punctatus, palecheek parrotfish, Scarus viridis, banded archerfish, Toxotes jaculator, blotched picarel, Maena vulgaris, gilthead seabream, Sparus aurata, climbing perch, Anabas scandens, colisa, Polyacanthus colisa, and giant gourami. Lithograph from Lorenz Oken's Universal Natural History, Allgemeine Naturgeschichte fur alle Stande, Stuttgart, 1841.

FLO4684911

White seabass

UIG531673

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not just any Seyfert galaxy; it is the second brightest Seyfert galaxy known. It is also the brightest and most dominant member of the Dorado Group, a loose concentration of galaxies that together comprise one of the richest galaxy groups of the southern hemisphere. This image highlights the beauty and awe-inspiring nature of this unique galaxy group, with NGC 1566 glittering and glowing, its bright nucleus framed by swirling and symmetrical lavender arms. This image was taken by Hubble's Wide Field Camera 3 (WFC3) in the near-infrared part of the spectrum — Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

PIX4609939

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