File:Delorme 1 (AB)b JWST MIRI IFU.jpg
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b_JWST_MIRI_IFU.jpg){kind=link}
Summary
| Description |
English: Delorme 1 system with the stellar binary at the bottom and the planet at the top. An molecular hydrogen outflow (here: violet) was discovered by Mâlin+2025.
JWST MIRI IFU channel 2 image (see MIRI MRS) I used channel 2 sub-bands short, medium and long (average in QFITSView) as RGB components and overlayed an image centered at H2 S(3) 9.665 Microns (see figure 8&9 of Mâlin+) in violet. The noise and stellar radiation at 9.665 Microns of the binary star (no H2 emission) was removed. program: GTO 2778 Principal Investigator: Marshall Perrin I created this image with QFITSView and Photoshop Elements |
| Date | |
| Source | Own work |
| Author | NASA/ESA/CSA JWST MIRI; Marshall Perrin et al. & Melina Thévenot |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 09:35, 9 October 2025 | | 780 × 716 (79 KB) | wikimediacommons>Meli thev | Uploaded own work with UploadWizard |
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b_JWST_MIRI_IFU.jpg){kind=link}