Astronomy and Space

CW Leonis

CW Leonis or IRC +10216 is a variable carbon star that is embedded in a thick dust envelope. It was first discovered in 1969 by a group of astronomers led by Eric Becklin, based upon infrared observations made with the 62-inch Caltech Infrared Telescope at Mount Wilson Observatory. Its energy is emitted mostly at infrared wavelengths. At a wavelength of 5 μm, it was found to have the highest flux of any object outside the Solar System.

Also on this shelf

See also

• ▸HD 80230
• ▸Arecibo Observatory
• ▸Delta Persei

Uncatalogued shelf

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