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PHOTO CAPTION>
The binary star system of BZ Cam, some 2,500 light-years distant toward Camelopardalis, is poorly understood. In a typical cataclysmic variable, matter expelled from the larger star accumulates on the white dwarf companion, ultimately causing a nova-like flare. BZ Cam, however, flickers irregularly, and expels a stellar wind that creates a bow-shockwave as the binary moves through the local interstellar medium. (R. Casalegno, C. Conselice, et al., WIYN, NOAO, MURST, and NSF.)
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