2009/08/01 by Y. C. Liang, Guo‐Hua Zhong, G. H. Zhong +10
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Brightness #Disc galaxy #Galaxies: Formation, Evolution, Phenomena #Galaxy #Luminous infrared galaxy #Physics #Stellar, planetary, and galactic studies #Surface brightness #Surface brightness fluctuation #astro-ph.CO
paper · pdf · doi:10.1017/s1743921310002802
published in Proceedings of the International Astronomical Union 5(S262), 213-216 (Cambridge University Press) · 4 pages, 2 figures, to appear in proceedings of IAU symposium 262, Stellar Populations: Planning for the Next Decade, eds. G. Bruzual & S. Charlot
openalex publication_date 2009/08/01 · arxiv created 2009/10/11 · arxiv updated 2015/05/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
Abstract A large sample of low surface brightness (LSB) disk galaxies is selected from SDSS with B-band central surface brightness μ 0 (B) from 22 to 24.5 mag arcsec −2 . Some of their properties are studied, such as magnitudes, surface brightness, scalelengths, colors, metallicities, stellar populations, stellar masses and multiwavelength SEDs from UV to IR etc. These properties of LSB galaxies have been compared with those of the galaxies with higher surface brightnesses. Then we check the variations of these properties following surface brightness.