Figure 12 from HAZMAT. III. The UV Evolution of Mid- to Late-M Stars with GALEX

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

HAZMAT. III. The UV Evolution of Mid- to Late-M Stars with GALEX

Authors: Adam C. Schneider, and Evgenya L. Shkolnik

2018 The Astronomical Journal 155 122.

Provider: AAS Journals

Caption: Figure 12.

Absolute FUV flux density vs. absolute NUV flux density for young (<50 Myr; left) and field-age (∼5 Gyr; right) low-mass stars. Black-lines represent least-squares fits to the data. For the field-age sample, we determine separate fits for higher-mass (>0.35 M_⊙) and lower-mass (≤0.35 M_⊙) Ms.

Other Images in This Article

Copyright and Terms & Conditions