A star with jets?Beta Lyrae Beta Lyrae (β Lyr / β Lyrae) is a binary star system approximately 882 light-years away in the constellation Lyra. Beta Lyrae is traditionally named Sheliak which is Arabic for "tortoise" or "harp. ranks as one of the most widely studied stars in the heavens. Historical observations of this binary system, which consists of one star that donates mass to a disk of material encircling encircling (en·serˑ·k a companion, date to 1785. Now, a shuttleborne telescope has given astronomers their first three-dimensional view of Beta Lyrae. The data hint that jets of hot gas squirt out of the poles of the star within the disk. Astronomers can't view the interior of Beta Lyrae directly because the disk blocks it, notes Kenneth H. Nordsieck of the University of Wisconsin-Madison “University of Wisconsin” redirects here. For other uses, see University of Wisconsin (disambiguation). A public, land-grant institution, UW-Madison offers a wide spectrum of liberal arts studies, professional programs, and student activities. . But gas lying above and below the poles of the central star polarizes light from Beta Lyrae, reflecting some of it toward Earth and enabling scientists to peek inside the binary system. In conjunction with ground-based observations of polarized A one-way direction of a signal or the molecules within a material pointing in one direction. visible light, data from the Wisconsin Ultraviolet Photopolarimeter Experiment, which flew aboard the Astro 2 Observatory last March, revealed the presence of such polar gas clouds. Nordsieck says that by analogy with much larger systems that have accretion disks, such as quasars Proper naming of quasars are by Catalogue Entry, Qxxxx±yy using B1950 coordinates, or QSO Jxxxx±yyyy using J2000 coordinates. This page lists quasars.
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