Figure 2 from First Detection of Ultraviolet Emission from a Detached Dust Shell: Galaxy Evolution Explorer Observations of the Carbon Asymptotic Giant Branch Star U Hya

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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 2.

FUV (top panel) and NUV (bottom panel) background-subtracted surface brightness radial profiles. Surface brightness axis is limited to highlight the extended emission near ~100'', bins closest to the central point source emission are indicated with upward pointing arrows because their emission lies beyond the plot range.

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