Using Colours to Determine the Stellar Ages and Metallicities of Distant Galaxies
The determination of stellar populations of galaxies are important for studying the formation and evolution of galaxies, because all galaxies contain many stars and they evolve with galaxies. Spectra data are usually used to determine the stellar populations of nearby galaxies as they have the ability to disentangle the de generacy between stellar age and metallicity. However, it is difficult to give similar studies to distant (e.g., Ζ > 0.3) galaxies because of the lack of reliable spectra data. This is actually limited by current observational equipments and methods. In fact, the information of the stellar ages and metallicities of distant galaxies are crucial for solving the problem of galaxy formation and evolution. Colours can give us some in formation of the stellar populations of distant galaxies. In the paper, I introduce our works about using colours to estimate the ages and metallicities of the stellar popu lations of galaxies. Some potential colours for studying stellarpopulation parameters (age and metallicity) and their sensitivities to stellar-population parameters are re viewed. A new composite stellar population model that includes both single stars and binary stars is also introduced.
galaxies stellar content galaxies evolution galaxies formation
Zhongmu Li
College of Physics and Electrical Information, Dali University, Dali, 671003, China
国际会议
The 10th Asian-Pacific Regional International Astronomical Union Meeting(第十届亚洲及太平洋地区天文学大会 APRIM)
昆明
英文
314-316
2008-08-03（万方平台首次上网日期，不代表论文的发表时间）