Figure 3 from First Detection of Ultraviolet Emission from a Detached Dust Shell: Galaxy Evolution Explorer Observations of the Carbon Asymptotic Giant Branch Star U Hya

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

First Detection of Ultraviolet Emission from a Detached Dust Shell: Galaxy Evolution Explorer Observations of the Carbon Asymptotic Giant Branch Star U Hya

Authors: Enmanuel Sanchez Rodolfo Montez, Jr., Sofia Ramstedt, and Keivan G. Stassun

Sanchez et al. 2015 The Astrophysical Journal Letters 798 L39.

Provider: AAS Journals

Caption: Figure 3.

Dust shell of U Hya observed by Herschel PACS in 70 μm band with contours of the GALEX FUV emission overlaid. The yellow contours correspond to the faint spoke-like feature discussed in Section 4.4. The proper motion vector is indicated along with the best-fit ellipse for the bright FUV points.

Other Images in This Article

Copyright and Terms & Conditions