Latest Images
V images are displayed in log scale, and FUV im...
The process of sky/background fitting and subtr...
As in Figure 2.
Reproduction of the integrated H I (moment 0) m...
PA and b/a of isophotes as a function of surfac...
As in Figure 2.
As in Figure 2.
Average stacked V image produced by summing sev...
Surface photometry of the stacked V image. The ...
Colors of annuli from the stacked images. Each ...
All images are shown with a logarithmic scale f...
As for Figure 11.
As for Figure 11. NGC 3738 is centrally concent...
The mass-loss picture of SN 2023fyq that we der...
Radio SEDs of SN 2023fyq at Δt ≈ 58–525 days. T...
Radio 10 GHz light curve of SN 2023fyq with var...
The unabsorbed X-ray light curves of the detect...
The peak spectral luminosity versus peak time f...
A view of all previous radio-observed SNe Ibn a...
Radio SEDs of SN 2023fyq at VLA frequencies (3–...
Temperature slices at t = 0.45 s of the equator...
The initial turbulent velocity (left) and magne...
Fraction of burnt material at three times, t = ...
Filling factors as a function of time. Shown is...
ANNOUNCEMENTS
Take the AstroExplorer for a spin!
Be sure to try the search and sorting features, which were added based on user feedback; browse and find the links to videos and interactive figures in our Journal articles; find AAS Research Notes; or notice that new publishers have begun adding their figures to the AIE. Get in touch to hear more!
