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Despite their high gas fractions, these are not low-surface-brightness galaxies and have typical specific star formation rates (SFR<jats:inline-formula>\n                     <jats:tex-math>\n\n<\/jats:tex-math>\n                     <jats:inline-graphic xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" xlink:href=\"ajaa436bieqn5.gif\" xlink:type=\"simple\"\/>\n                  <\/jats:inline-formula>) for their stellar masses. The three galaxies have normal SFRs for their <jats:inline-formula>\n                     <jats:tex-math>\n\n<\/jats:tex-math>\n                     <jats:inline-graphic xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" xlink:href=\"ajaa436bieqn6.gif\" xlink:type=\"simple\"\/>\n                  <\/jats:inline-formula> masses, but unusually short star formation efficiency scale lengths, indicating that the star formation bottleneck in these galaxies is in the conversion of <jats:inline-formula>\n                     <jats:tex-math>\n\n<\/jats:tex-math>\n                     <jats:inline-graphic xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" xlink:href=\"ajaa436bieqn7.gif\" xlink:type=\"simple\"\/>\n                  <\/jats:inline-formula> to <jats:inline-formula>\n                     <jats:tex-math>\n\n<\/jats:tex-math>\n                     <jats:inline-graphic xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" xlink:href=\"ajaa436bieqn8.gif\" xlink:type=\"simple\"\/>\n                  <\/jats:inline-formula>, not in converting <jats:inline-formula>\n                     <jats:tex-math>\n\n<\/jats:tex-math>\n                     <jats:inline-graphic xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" xlink:href=\"ajaa436bieqn9.gif\" xlink:type=\"simple\"\/>\n                  <\/jats:inline-formula> to stars. 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