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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2403.03872 |
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| _version_ | 1866917875196887040 |
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| author | Juodžbalis, Ignas Maiolino, Roberto Baker, William M. Tacchella, Sandro Scholtz, Jan D'Eugenio, Francesco Schneider, Raffaella Trinca, Alessandro Valiante, Rosa DeCoursey, Christa Curti, Mirko Carniani, Stefano Chevallard, Jacopo de Graaff, Anna Arribas, Santiago Bennett, Jake S. Bourne, Martin A. Bunker, Andrew J. Charlot, Stéphane Jiang, Brian Koudmani, Sophie Perna, Michele Robertson, Brant Sijacki, Debora Übler, Hannah Williams, Christina C. Willott, Chris Witstok, Joris |
| author_facet | Juodžbalis, Ignas Maiolino, Roberto Baker, William M. Tacchella, Sandro Scholtz, Jan D'Eugenio, Francesco Schneider, Raffaella Trinca, Alessandro Valiante, Rosa DeCoursey, Christa Curti, Mirko Carniani, Stefano Chevallard, Jacopo de Graaff, Anna Arribas, Santiago Bennett, Jake S. Bourne, Martin A. Bunker, Andrew J. Charlot, Stéphane Jiang, Brian Koudmani, Sophie Perna, Michele Robertson, Brant Sijacki, Debora Übler, Hannah Williams, Christina C. Willott, Chris Witstok, Joris |
| contents | Recent observations have found a large number of supermassive black holes already in place in the first few hundred million years after Big Bang. The channels of formation and growth of these early, massive black holes are not clear, with scenarios ranging from heavy seeds to light seeds experiencing bursts of high accretion rate. Here we present the detection, from the JADES survey, of broad Halpha emission in a galaxy at z=6.68, which traces a black hole with mass of ~ 4 * 10^8 Msun and accreting at a rate of only 0.02 times the Eddington limit. The host galaxy has low star formation rate (~ 1 Msun/yr, a factor of 3 below the star forming main sequence). The black hole to stellar mass ratio is ~ 0.4, i.e. about 1,000 times above the local relation, while the system is closer to the local relations in terms of dynamical mass and velocity dispersion of the host galaxy. This object is most likely the tip of the iceberg of a much larger population of dormant black holes around the epoch of reionisation. Its properties are consistent with scenarios in which short bursts of super-Eddington accretion have resulted in black hole overgrowth and massive gas expulsion from the accretion disk; in between bursts, black holes spend most of their life in a dormant state. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_03872 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | A dormant, overmassive black hole in the early Universe Juodžbalis, Ignas Maiolino, Roberto Baker, William M. Tacchella, Sandro Scholtz, Jan D'Eugenio, Francesco Schneider, Raffaella Trinca, Alessandro Valiante, Rosa DeCoursey, Christa Curti, Mirko Carniani, Stefano Chevallard, Jacopo de Graaff, Anna Arribas, Santiago Bennett, Jake S. Bourne, Martin A. Bunker, Andrew J. Charlot, Stéphane Jiang, Brian Koudmani, Sophie Perna, Michele Robertson, Brant Sijacki, Debora Übler, Hannah Williams, Christina C. Willott, Chris Witstok, Joris Astrophysics of Galaxies Recent observations have found a large number of supermassive black holes already in place in the first few hundred million years after Big Bang. The channels of formation and growth of these early, massive black holes are not clear, with scenarios ranging from heavy seeds to light seeds experiencing bursts of high accretion rate. Here we present the detection, from the JADES survey, of broad Halpha emission in a galaxy at z=6.68, which traces a black hole with mass of ~ 4 * 10^8 Msun and accreting at a rate of only 0.02 times the Eddington limit. The host galaxy has low star formation rate (~ 1 Msun/yr, a factor of 3 below the star forming main sequence). The black hole to stellar mass ratio is ~ 0.4, i.e. about 1,000 times above the local relation, while the system is closer to the local relations in terms of dynamical mass and velocity dispersion of the host galaxy. This object is most likely the tip of the iceberg of a much larger population of dormant black holes around the epoch of reionisation. Its properties are consistent with scenarios in which short bursts of super-Eddington accretion have resulted in black hole overgrowth and massive gas expulsion from the accretion disk; in between bursts, black holes spend most of their life in a dormant state. |
| title | A dormant, overmassive black hole in the early Universe |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2403.03872 |