File:Disks in the Sigma Ori Cluster as seen by ALMA.jpg
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Summary
| Description |
English: Images captured by ALMA's most extended antenna configuration reveal surprisingly rich disk structures in the Sigma Ori cluster.
Additional information from Huang et al. 2024, see figure 3 and table 1: Source names from left to right top row: SO 1152 (M0-type star, 2MASS J05393938–0217045, Haro 5-25), SO 1274 (K7-type star, 2MASS J05395465–0246341, Haro 5-34), SO 1153 (K5-type star, 2MASS J05393982–0231218, Haro 5-27), SO 844 (M1-type star, 2MASS J05390136–0218274, Haro 5-16) Source names from left to right bottom row: SO 1036 (M0-type star, 2MASS J05392519–0238220, V* BG Ori), SO 984 (K7-type star, 2MASS J05391883–0230531, Haro 5-21), SO 897 (K6-type star, 2MASS J05390760–0232391, Haro 5-19), SO 662 (K7-type star, 2MASS J05384027–0230185, Haro 5-13) |
| Date | |
| Source | https://www.almaobservatory.org/en/press-releases/alma-reveals-planets-can-form-under-harsh-radiation/ |
| Author | ALMA (ESO/JAO/NAOJ/NRAO), J. Huang et. al. |
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