File:Classical Be star.jpg
![File:Classical Be star.jpg](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d8/Classical_Be_star.jpg/756px-Classical_Be_star.jpg?20100916115156)
Size of this preview: 756 × 600 pixels. Other resolutions: 303 × 240 pixels | 605 × 480 pixels | 1,000 × 793 pixels.
Original file (1,000 × 793 pixels, file size: 83 KB, MIME type: image/jpeg)
File information
Structured data
Captions
Captions
Add a one-line explanation of what this file represents
Summary
editDescriptionClassical Be star.jpg |
English: Life near the double-star system of Phi Persei is never dull, as this illustration shows. Taken from the perspective of one of the Hubble Space Telescope observations of Phi Persei, this artist's depiction provides a taste of the double- star system's unstable existence. The bright "Be" star - a type of hot star with a broad, flattened disk - is the white, semicircular object looming in the upper right of the illustration. The red, pancake-shaped object surrounding the star is a gas disk. The gas is material the star is losing because of its rapid rotation. The small, hot subdwarf is in the lower left of the illustration. The blasts of white light represent particles of material - called a stellar wind - being released by the star. This powerful stellar wind is heating part of the "Be" star's gas disk. The red ring of material surrounding the subdwarf was probably formed from the "Be" star's outflow of gas. The subdwarf is moving toward the right in its 126-day orbit around the "Be" star. |
||||
Source | http://hubblesite.org/newscenter/archive/releases/1997/39/image/a/ | ||||
Author | Bill Pounds | ||||
Permission (Reusing this file) |
|
Licensing
edit![w:en:Creative Commons](https://upload.wikimedia.org/wikipedia/commons/thumb/7/79/CC_some_rights_reserved.svg/90px-CC_some_rights_reserved.svg.png)
![attribution](https://upload.wikimedia.org/wikipedia/commons/thumb/1/11/Cc-by_new_white.svg/24px-Cc-by_new_white.svg.png)
![share alike](https://upload.wikimedia.org/wikipedia/commons/thumb/d/df/Cc-sa_white.svg/24px-Cc-sa_white.svg.png)
This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
- share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 11:51, 16 September 2010 | ![]() | 1,000 × 793 (83 KB) | Sadalsuud~commonswiki (talk | contribs) | {{Information |Description={{en|1=Life near the double-star system of Phi Persei is never dull, as this illustration shows. Taken from the perspective of one of the Hubble Space Telescope observations of Phi Persei, this artist's depiction provides a tast |
You cannot overwrite this file.
File usage on Commons
The following page uses this file:
File usage on other wikis
The following other wikis use this file:
- Usage on en.wikipedia.org
- Usage on ja.wikipedia.org
- Usage on ko.wikipedia.org
- Usage on zh.wikipedia.org
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
_error | 0 |
---|