Your selection
Clear selectionLeave the work to our dedicated Account Managers.
Item added to cart
Find Your Perfect Match The top results are exact matches, while the rest are visually similar images curated from our archive.
Drag file here
Upload
Processing search results
Waiting for update..
Error:
Searching for a particular field
| Field | Search term | Example |
| Asset title | title: | title:pony |
| Asset title and keywords | ~ | ~pony |
| Asset description text | description: | description:london |
| Agency prefix | prfx: or $ | prfx:lal or $LAL |
| Asset id | imageid: or # | imageid:250297 or imageid:[2500 TO 4000] or #1551 |
| Agency name | coll: | coll:history |
| Medium | medium: | medium:oil |
| Century | century: | century:20th |
| Keywords | kw: | kw:dog |
| Artist name | artist: or ? | artist:monet or ?monet |
| Artist nationality | nat: | nat:French |
| Creator ID | creatorid: | creatorid:37 |
| Location | loc: or @ | loc:exeter or @exeter |
| Classification | class: | class:57 or #57. Use # for unclassified assets |
| Year | year: | year:1850 or year:[1700 TO 1800] |
AVE8905382
Chris Caldicott
CDT6375898
Chris Caldicott
CDT6375898
Chris Caldicott
CDT6375899
Chris Caldicott
CDT6375899
![Remnants of Supernova of Vails - detail - Pencil Nebula (NGC 2376) - Remnants from a star that exploded thousands of years ago created a celestial abstract portrait, as captured in this image of the Pencil Nebula. Officially known as NGC 2736, the Pencil Nebula is part of the huge Vela supernova remnant, located in the southern constellation Vela. Discovered by Sir John Herschel in the 1840s, the nebula's linear appearance triggered its popular name. The nebula's shape suggests that it is part of the supernova shock wave that recently encountered a region of dense gas. It is this interaction that causes the nebula to glow, appearing like a rippled sheet. In this snapshot, astronomers are looking along the edge of the undulating sheet of gas. This view shows large, wispy filamentary structures, smaller bright knots of gas, and patches of diffuse gas. The Hubble Heritage Team used the Advanced Camera for Surveys in October 2002 to observe the nebula. The region of the Pencil Nebula captured in this image is about three fourths of a light - year across. The Vela supernova remnant is 114 light - years (35 parsecs) across. The remnant is about 815 light - years (250 parsecs) away from our solar system. The nebula's luminous appearance comes from dense gas regions that have been struck by the supernova shock wave. As the shock wave travels through space [from right to left in the image], it rams into interstellar material. Initially the gas is heated to millions of degrees, but then subsequently cools down, emitting the optical light visible in the image. The colors of the various regions in the nebula yield clues about this cooling process. Some regions are still so hot that the emission is dominated by ionized oxygen atoms, which glow blue in the picture. Other regions have cooled more and are seen emitting red in the image (cooler hydrogen atoms). In this situation, color shows the temperature of the gas. The nebula is visible in this image because it is glowing](https://images-cdn.bridgemanimages.com/api/1.0/image/600wm.PIX.89958540.7055475/4582819.jpg?old-wm)
We partner with the world's leading museums, galleries and artists, so you have access to the highest-quality imagery.
Our teams can help you find the perfect content and take care of all of the copyright and licensing requirements.
Bridgeman Images
77 Sands Street, 6th Floor
Brooklyn, NY 11201
United States
T: +1 212 828 1238
© Copyright 2025 Bridgeman Art Library Limited. Registered in England and Wales as company number 01056394.
