The Giant Proto-galaxy Cb58; an Artifact of Gravitational Lensing ? Publication Manuscript

نویسندگان

  • L. L. R. Williams
  • G. F. Lewis
چکیده

The proto-galaxy, cB58, was discovered in the CNOC survey of cluster redshifts. Absorption features reveal that this system is at a redshift of z = 2 : 72, implying an absolute magnitude of M v 26, and a star-formation rate of 4700M yr 1 , making it the most \active" star-forming galaxy. This proto-galaxy is observed to lie close (6 00) to a central cluster galaxy at z = 0 : 373. The X-ray properties of the cluster suggests that its mass, and therefore its lensing potential, could be greater than that found using a virial analysis. In this Letter we argue that the phenomenal properties of this proto-galaxy are due to the gravitational lensing eect of the foreground cluster, and the unlensed properties of the source are typical of high-redshift star-forming systems.

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تاریخ انتشار 1996