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Session 83 - Starbursts and Mergers.
Oral session, Thursday, June 13
We present follow-up observations of the proto-galaxy candidate MS1512-cB58 at z=2.72 discovered by Yee et al. (1996). cB58 is an extremely luminous, well-resolved disk-like galaxy, with a rest UV spectrum containing strong P-Cygni lines indicative of the presence of massive O and B stars. The spectral energy distribution from rest frame 1300-6000 Å\ is fit by population synthesis models from Bruzual and Charlot (1993) which confirm a very young age for this galaxy. While a substantial older population cannot be completely ruled out with the present data, the simplest interpretation is that this is a galaxy within about 100 million years of the initial burst of star-formation which created most of its stellar mass, and that it will likely evolve into a bright galaxy of several L* by today. Observations to further constrain the star formation rate, dust mass, molecular mass, and limit the extent to which it is gravitationally lensed by foreground objects will be discussed.
Program listing for Thursday