Fig. 7 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.

Provider: AAS Journals

Caption: Fig. 7.

Velocity of ISM and stellar lines of NGC 1705‐1 vs. lower ionization potential. Symbols as in Fig. 6. The point at (16.35, −14) denotes the two Si III lines at 1297 and 1343 Å, for which we measured the same velocity. The lowest velocity value for the stellar lines corresponds to the faint Si II line at 1533 Å.

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