IRC +10216
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. IRC +10216 or CW Leonis is a well-studied 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 inches Caltech Infrared Telescope at Mount Wilson Observatory. Its energy is emitted mostly at infrared wavelengths. At a wavelength of 5 m, it was found to have the highest flux of any object outside the Solar System.

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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. IRC +10216 or CW Leonis is a well-studied 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 inches Caltech Infrared Telescope at Mount Wilson Observatory. Its energy is emitted mostly at infrared wavelengths. At a wavelength of 5 m, it was found to have the highest flux of any object outside the Solar System.