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Summary
| Description |
English: https://arxiv.org/abs/1907.02538
According to Pinte et al. 2019, the "kink" in the velocity of the CO gas on the surface of the disk is caused by a protoplanet, which is still embedded into the protoplanetary disk around the star HD 97048. The protoplanet is also responsible for the gap in the dusty part of the disk, which maps the midplane of the disk. |
| Date | |
| Source | https://figshare.com/articles/dataset/HD_97048_ALMA_B7_continuum_13CO/8266988 |
| Author | ALMA - Pinte et al. 2019 - adapted and mixed by Meli_thev |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 19:46, 1 March 2023 | | 1,400 × 1,436 (501 KB) | Meli thev | Uploaded a work by ALMA - Pinte et al. 2019 - adapted and mixed by Meli_thev from https://figshare.com/articles/dataset/HD_97048_ALMA_B7_continuum_13CO/8266988 with UploadWizard |
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