Structural Characteristics and Stellar Composition of Low Surface Brightness Disk Galaxies

We presentUBV I surface photometry of a sample of low surface brightness (LSB) disk galaxies. LSB disk galaxies are fairly well described as exponential disks with no preferred value for either scale length, central surface brightness, or rotational velocity. Indeed, the distribution of scale lengths is indistinguishable from that of high surface brightness spirals, indicating that dynamically similar galaxies (e.g., those with comparable v 2 R) exist over a large range in surface density. These LSB galaxies are strikingly blue. The complete lack of correlation between central surface brightness and color rules out any fading scenario. Similarly, the oxygen abundances inferred from H II region spectra are uncorrelated with color so the low metallicities are not the primary cause of the blue colors. While these are di cult to interpret in the absence of signi cant star formation, the most plausible scenario is a stellar population with a young mean age stemming from late formation and subsequent slow evolution. These properties suggest that LSB disks formed from low initial overdensities with correspondingly late collapse times. Subject headings: galaxies: evolution | galaxies: formation | galaxies: stellar content | galaxies: structure