Fig. 8 from SBS 0335−052, A Probable Nearby Young Dwarf Galaxy: Evidence Pro and Con

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SBS 0335−052, A Probable Nearby Young Dwarf Galaxy: Evidence Pro and Con

Authors: Yuri I. Izotov, Valentin A. Lipovetsky, Frederic H. Chaffee, Craig B. Foltz, Natalia G. Guseva, and Alexei Y. Kniazev

Izotov et al. 1997 The Astrophysical Journal 476 698.

Provider: AAS Journals

Caption: Fig. 8.

Fragment of the SBS 0335−052 spectrum, showing the presence of a low‐intensity, broad component of the Hβ λ4861 emission line with FWZI ~50 Å. Note that the He II λ4686 emission line is narrow, implying its nebular origin.

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