Fig. 14 from Characterizing the Stellar Population in NGC 1705‐1

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Characterizing the Stellar Population in NGC 1705‐1

Authors: Gerardo A. Vázquez, Claus Leitherer, Timothy M. Heckman, Danny J. Lennon, Duília F. de Mello, Gerhardt R. Meurer, and Crystal L. Martin

Vázquez et al. 2004 The Astrophysical Journal 600 162.

Caption: Fig. 14.

Merged FUSE and HST/STIS spectra of NGC 1705‐1. The smooth curve is a power‐law fit to the observed spectra with an exponent of ﹩\beta =-2.5﹩.