There has been considerable progress in recent years in determining stellar masses of galaxies. In this talk, I discuss various methods and their uncertainties. In particular, I will discuss the stellar masses that one can obtain from near-infrared imaging and spectroscopy, through stellar population synthesis.
Primary Language | English |
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Subjects | Astronomical Sciences (Other) |
Journal Section | Conference Paper |
Authors | |
Publication Date | December 11, 2020 |
Submission Date | September 18, 2015 |
Published in Issue | Year 2020 Volume: 1 Issue: 1 |
TJAA is a publication of Turkish Astronomical Society (TAD).