A jetted wandering massive black hole candidate in a dwarf galaxy
Dwarf galaxies, with their shallow gravitational potentials, less evolved assembly histories, and low mass, serve as critical laboratories for studying massive black hole (MBH) formation and growth. They preserve signatures of the primordial processes that shaped early MBH emergence.
Authors
- Tao An (ORCID: https://orcid.org/0000-0003-4341-0029)
- Yingkang Zhang (ORCID: https://orcid.org/0000-0001-8256-8887)
- Jun Yang (ORCID: https://orcid.org/0000-0002-2322-5232)
- Yuanqi Liu (ORCID: https://orcid.org/0000-0001-9321-6000)
- Ailing Wang (ORCID: https://orcid.org/0000-0002-7351-5801)
- Xiaopeng Cheng (ORCID: https://orcid.org/0000-0003-4909-2682)
- Mar Mezcua
Institutions
- Chinese Academy of Sciences (CN)
- Shanghai Astronomical Observatory (CN)
- Korea Astronomy and Space Science Institute (KR)
- Institut d'Estudis Espacials de Catalunya (ES)
- Institute of High Energy Physics (CN)
- Chalmers University of Technology (SE)
- Universitat Politècnica de Catalunya (ES)
Publication Details
- Journal
- Science Bulletin
- Published
- 2025-09-04
- DOI
- https://doi.org/10.1016/j.scib.2025.09.001
- Primary Topic
- Astrophysical Phenomena and Observations
- Type
- article
- Field-Weighted Citation Impact
- 0.00