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Summary
| Description |
English: An annotated false-color image of the WISPIT 2 system as seen in infrared light (L' bandpass, ~3.7 micron wavelength) by the Large Binocular Telescope Interferometer (LBTI) and the L- and M-band InfraRed Camera (LMIRcam). The host star has been subtracted from the center of the image, with the inner lambda/D radius masked. Two bright circumstellar point sources are seen: CC1 - a superjovian protoplanet candidate in the inner disk cavity, and b - a superjovian protoplanet in a more distant gap in the disk. Three protoplanetary disk rings are visible despite self-subtraction from the KLIP-ADI algorithm (Rings 1, 2, and 3 in R. van Capelleveen et al. 2025).
The underlying image is identical to that of Figure 2 of Close, van Capelleveen, Weible et al. 2025, but upsampled and shown with a different colormap and an asinh stretch. Link to the paper published in ApJL: https://iopscience.iop.org/article/10.3847/2041-8213/adf7a5 |
| Date | |
| Source | Own work |
| Author | Laird Close & Gabriel Weible (University of Arizona) |
Licensing
I, the copyright holder of this work, hereby publish it under the following license:
This file is licensed under the Creative Commons Attribution 4.0 International license.
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File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:16, 26 August 2025 | | 2,030 × 2,030 (1.59 MB) | GabrielWeible | Uploaded own work with UploadWizard |
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