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Hα Velocity Fields of H II Regions in Nearby Dwarf Irregular Galaxies

  • Authors: Akihiko Tomita, Kouji Ohta, Kouichiro Nakanishi, Tsutomu T. Takeuchi, and Mamoru Saitō

Tomita et al. 1998 The Astronomical Journal 116 131.

  • Provider: AAS Journals

Caption: Fig. 1.

Slit positions superposed on the Hα images. The length of each line corresponds to the length of the abscissa in Fig. 2. (a) NGC 2366: the Hα image is taken from Fig. 1 in Roy et al. (1991). The length of the line corresponds to 160﹩\arcsec﹩. (b) Holmberg II: the Hα image is taken from Fig. 1 in Hodge et al. (1994). The length of the line corresponds to 250﹩\arcsec﹩. (c) IC 2574: the Hα image is taken from Fig. 3 in Miller & Hodge (1994). The length of the line corresponds to 200﹩\arcsec﹩. (d) WLM: the Hα image is taken from Fig. 1a in Hodge & Miller (1995). The length of the line corresponds to 200﹩\arcsec﹩.
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