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37 L 8 sec. Combining this constraint with the dynamical mass limit derived from the CO kinematics, Scoville, Yun & Bryant (1995) find that ml = 5 M 8 , mu = 23 M 8 , and M = 90M8 yr- 1 (with a burst timescale of 5 X 10 7 yr). The narrow range of permissable stellar masses suggests that a starburst origin for a major fraction of the luminosity in Arp 220 is unlikely, although not ruled out. lM8 ) are categorically ruled out since they violate the L / M* constraint by more than an order of magnitude; similarly starbursts with only high mass OB stars are easily ruled out since they violate the L/Q constraint.

Griffiths, R. et al. 1995, ApJ, in press. Henkel, C. L. 1990, A&A 229, 43l. L. and Biermann, P. 1984, A&A 141, Ll. E. and Withington, S. 1994, MNRAS 269, L28. Katz, N. et al. 1995 ApJ, in press. , Padmanabhan, T. and Subramanian, K. 1995, MNRAS 272, 54. J. and Guilloteau, S. 1993, A&A 280, L3. Lilly, S. et al. 1995, ApJ, in press. COLD GAS AT HIGH REDSHIFT 21 McCarthy, P. 1989 PhD Thesis, UC Berkeley. , Kreysa, E. T. 1994, MNRAS 267, L9. Meylan, G. 1995, QSO Absorption Lines (Springer). Illler, P.

And Withington, S. 1994, MNRAS 269, L28. Katz, N. et al. 1995 ApJ, in press. , Padmanabhan, T. and Subramanian, K. 1995, MNRAS 272, 54. J. and Guilloteau, S. 1993, A&A 280, L3. Lilly, S. et al. 1995, ApJ, in press. COLD GAS AT HIGH REDSHIFT 21 McCarthy, P. 1989 PhD Thesis, UC Berkeley. , Kreysa, E. T. 1994, MNRAS 267, L9. Meylan, G. 1995, QSO Absorption Lines (Springer). Illler, P. et al. 1995, ApJ, in preparation. , Katz, N. and Lake, G. 1995, ApJ, in press. S. M. 1995, MNRAS 275, 56. J. C. 1995, MNRAS, in press.

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