File:HD 97048 disk.png
Size of this preview: 584 × 599 pixels. Other resolutions: 234 × 240 pixels | 468 × 480 pixels | 749 × 768 pixels | 998 × 1,024 pixels | 1,400 × 1,436 pixels.
Original file (1,400 × 1,436 pixels, file size: 501 KB, MIME type: image/png)
 | This is a file from the Wikimedia Commons. Information from its description page there is shown below. Commons is a freely licensed media file repository. You can help. |
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 |
Licensing
This file is licensed under the Creative Commons Attribution 4.0 International license.
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
File history
Click on a date/time to view the file as it appeared at that time.
| 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 |
File usage
The following page uses this file:
Global file usage
The following other wikis use this file:
- Usage on zh-two.iwiki.icu
