File:Betelgeuse radio.jpg

Betelgeuse_radio.jpg(236 × 236 pixels, file size: 6 KB, MIME type: image/jpeg)

Summary edit

The asymmetric structure of Betelgeuse in radio waves is likely due to activity in the outer atmosphere of the star.

Licensing edit

Description

The asymmetric structure of Betelgeuse in radio waves is likely due to activity in the outer atmosphere of the star.

Source

The image appears on a website entitled, "Betelgeuse (Red giant)" at url=http://hubblesite.org/explore_astronomy/black_holes/encyc_mod1_q5.html.

Date

31 December 2015 (upload date)

Author

NRAO/AUI

Rationale

No free use or Public Domain image known to show the asymmetric structure of Betelgeuse in radio waves is likely due to activity in the outer atmosphere of the star. Per NRAO/AUI restriction to education, teaching and research. Commons checked.

Permission

Fair Use

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File history

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Date/TimeThumbnailDimensionsUserComment
current23:44, 31 December 2015Thumbnail for version as of 23:44, 31 December 2015236 × 236 (6 KB)Marshallsumter (discuss | contribs)The asymmetric structure of Betelgeuse in radio waves is likely due to activity in the outer atmosphere of the star. Category:Stars images

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