Fig. 4 from Mass Segregation and the Initial Mass Function of Super Star Cluster M82‐F

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Mass Segregation and the Initial Mass Function of Super Star Cluster M82‐F

Authors: Nate McCrady, James R. Graham, and William D. Vacca

McCrady, Graham, & Vacca 2005 The Astrophysical Journal 621 278.

Provider: AAS Journals

Caption: Fig. 4.

Measured half‐light radius and observed axial ratio as a function of wavelength. Lines are presented as a guide to the eye. The general decrease in size with wavelength is consistent with mass segregation. Note that the axial ratio remains constant within the error for all wavelengths other than 250 nm.

Other Images in This Article

Copyright and Terms & Conditions