Star formation powers optical line emission from the CGM.

Zhang H, Xie L, Qu Z, Zaritsky D, Ho LC, Bao M, Fontanot F, Hirschmann M, Liu C, De Lucia G, Wang E, Zheng H

DOI: 10.1126/sciadv.aec3939
Published: 2026 Sep 18
Container: Science advances
Publisher: Not recorded
Open access: yes

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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 = {Zhang H and Xie L and Qu Z and Zaritsky D and Ho LC and Bao M and Fontanot F and Hirschmann M and Liu C and De Lucia G and Wang E and Zheng H},
  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  - Zhang H
AU  - Xie L
AU  - Qu Z
AU  - Zaritsky D
AU  - Ho LC
AU  - Bao M
AU  - Fontanot F
AU  - Hirschmann M
AU  - Liu C
AU  - De Lucia G
AU  - Wang E
AU  - Zheng H
PY  - 2026
JO  - Science advances
DO  - 10.1126/sciadv.aec3939
UR  - https://doi.org/10.1126/sciadv.aec3939
ER  -

APA

H, Z., L, X., Z, Q., D, Z., LC, H., M, B., F, F., M, H., C, L., G, D. L., E, W., & H, Z. (2026). Star formation powers optical line emission from the CGM.. Science advances. https://doi.org/10.1126/sciadv.aec3939

Source records

pubmed · retrieved 2026-11-10T06:06:39.991Z