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Images of 'Filamentous' found, 10

scanning electron micrograph (SEM) depicts filamentous Ebola virus particles

scanning electron micrograph (SEM) depicts filamentous Ebola virus particles

UIG1578989

States of Mind (I) - Those who Stay or Study for 'States of Mind' or 'Those who Stay' or States of Mind (I) - Those who Stay (Stati d'animo (I) - Quelli che restano), by Umbero Boccioni, 1911, 20th Century, oil on canvas, 71 x 96 cm

States of Mind (I) - Those who Stay or Study for 'States of Mind' or 'Those who Stay' or States of Mind (I) - Those who Stay (Stati d'animo (I) - Quelli che restano), by Umbero Boccioni, 1911, 20th Century, oil on canvas, 71 x 96 cm

Boccioni, Umberto (1882-1916)

Luca Carrà

ELC850067

Silver

Silver

NHM1452926

Patches of encrusting red and green algae lie beneath filamentous bacterial mats on rock surfaces

Patches of encrusting red and green algae lie beneath filamentous bacterial mats on rock surfaces

UIG3524604

Patches of encrusting red and green algae lie beneath filamentous bacterial mats on rock surfaces

Patches of encrusting red and green algae lie beneath filamentous bacterial mats on rock surfaces

UIG3520305

Moths of the family Saturniidae

Moths of the family Saturniidae

NHM1452605

Paleontology. Filamentous acanthonemus (Acanthonemus filamentosus) fossil fish. In “Dictionnaire universel d'Histoire naturelle” by Mr. Charles D'Orbigny, 1841-1849.

Paleontology. Filamentous acanthonemus (Acanthonemus filamentosus) fossil fish. In “Dictionnaire universel d'Histoire naturelle” by Mr. Charles D'Orbigny, 1841-1849.

Jaime Abecasis

JAB5036794

Seahorse, Hippocampus, Filamentous Seahorse and greater pipefish, Syngnathus acus, Syngnathe needle. Handcoloured copperplate stipple engraving from Jussieu's “” Dictionary of Natural Sciences”” 1816-1830. The volumes on fish and reptiles were edited by Hippolyte Cloquet, natural historian and doctor of medicine. Illustration by J.G. Pretre, engraved by Massard, directed by Turpin, and published by F. G. Levrault.

Seahorse, Hippocampus, Filamentous Seahorse and greater pipefish, Syngnathus acus, Syngnathe needle. Handcoloured copperplate stipple engraving from Jussieu's “” Dictionary of Natural Sciences”” 1816-1830. The volumes on fish and reptiles were edited by Hippolyte Cloquet, natural historian and doctor of medicine. Illustration by J.G. Pretre, engraved by Massard, directed by Turpin, and published by F. G. Levrault.

FLO4644693

Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova Kepler in Ophiuchus - Kepler's supernova remnant — Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova K

Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova K

PIX4626476

The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both bright and dark filamentary clouds can be seen, many of which harbor stellar nurseries. The plane of the Milky Way's flat disk is apparent as the main, horizontal band of clouds. The brightest white spot in the middle is the very center of the galaxy, which also marks the site of a supermassive black hole. The region pictured here is immense, with a horizontal span of 890 light-years and a vertical span of 640 light-years. Earth is located 26,000 light-years away, out in one of the Milky Way's spiral arms. Though most of the objects seen in this image are located at the galactic center, the features above and below the galactic plane tend to lie closer to Earth. This image is a mosaic of thousands of short exposures taken by Spitzer's Infrared Array Camera. The entire region was imaged in less than 16 hours — The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both brig

The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both brig

PIX4637936

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