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Adhara
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Adhara

Binary star about 430 light years from Earth. The surface temperature of its brighter component, Adhara A, is 21,000 K (20,700°C/37,292°F), almost four times that of the Sun. Adhara's apparent magnitude is 1.5, so it can be regarded as the least bright of the first-magnitude stars or the brightest of the second-magnitude stars. It appears to us as the brightest source of extreme ultraviolet radiation in the sky, apart from the Sun.

Most of space contains un-ionized hydrogen in tiny amounts but Adhara is connected to our local cloud by a tunnel of almost hydrogen-free space. This means its ionizing radiation reaches our local cloud without obstruction. US astronomers concluded in 1995 that it plays a greater part in ionizing hydrogen in our region of the Galaxy than all the other 3 million stars lying closer to our local cloud.



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Cassinelli and colleagues at Wisconsin, the University of California at Berkeley, and Oxford University observed the relatively young, hot star Epsilon Canis Majoris in an attempt to uncover the energetic forces that drive stellar winds.
 
 
 
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