Star formation powers optical line emission from the CGM
- DOI
- 10.1126/sciadv.aec3939
- Published
- 2026-09-18
- Container
- Science Advances
- Publisher
- American Association for the Advancement of Science (AAAS)
- Open access
- unknown
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Cite this work
BibTeX
@article{allodium:10.1126/sciadv.aec3939,
title = {Star formation powers optical line emission from the CGM},
author = {Huanian Zhang and Lizhi Xie and Zhijie Qu and Dennis Zaritsky and Luis C. Ho and Min Bao and Fabio Fontanot and Michaela Hirschmann and Chenxu Liu and Gabriella De Lucia and Enci Wang and Haoyan Zheng},
year = {2026},
journal = {Science Advances},
doi = {10.1126/sciadv.aec3939},
url = {https://doi.org/10.1126/sciadv.aec3939}
}RIS
TY - JOUR TI - Star formation powers optical line emission from the CGM AU - Huanian Zhang AU - Lizhi Xie AU - Zhijie Qu AU - Dennis Zaritsky AU - Luis C. Ho AU - Min Bao AU - Fabio Fontanot AU - Michaela Hirschmann AU - Chenxu Liu AU - Gabriella De Lucia AU - Enci Wang AU - Haoyan Zheng PY - 2026 JO - Science Advances DO - 10.1126/sciadv.aec3939 UR - https://doi.org/10.1126/sciadv.aec3939 ER -
APA
Zhang, H., Xie, L., Qu, Z., Zaritsky, D., Ho, L. C., Bao, M., Fontanot, F., Hirschmann, M., Liu, C., Lucia, G. D., Wang, E., & Zheng, H. (2026). Star formation powers optical line emission from the CGM. Science Advances. https://doi.org/10.1126/sciadv.aec3939
Source records
- crossref · retrieved 2026-09-24T20:39:33.550Z