File:HD 97048 disk.png

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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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Captions

HD 97048 disk, dust and gas, showing a velocity kink caused by a protoplanet

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1 March 2023

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current19:46, 1 March 2023Thumbnail for version as of 19:46, 1 March 20231,400 × 1,436 (501 KB)Meli thevUploaded 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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