Signatures of star formation inside galactic outflows
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arXiv
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| Main Authors: | , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866917139234947072 |
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| author | Ong, Dily Duan Yi D'Eugenio, Francesco Maiolino, Roberto Arribas, Santiago Belfiore, Francesco Bellocchi, Enrica Carniani, Stefano Cazzoli, Sara Cresci, Giovanni Fabian, Andrew Ishibashi, Wako Mannucci, Filippo Marconi, Alessandro Russell, Helen Sturm, Eckhard Venturi, Giacomo |
| author_facet | Ong, Dily Duan Yi D'Eugenio, Francesco Maiolino, Roberto Arribas, Santiago Belfiore, Francesco Bellocchi, Enrica Carniani, Stefano Cazzoli, Sara Cresci, Giovanni Fabian, Andrew Ishibashi, Wako Mannucci, Filippo Marconi, Alessandro Russell, Helen Sturm, Eckhard Venturi, Giacomo |
| contents | Observations have suggested that galactic outflows contain substantial amounts of dense and clumpy molecular gas, creating favourable conditions for igniting star formation. Indeed, theoretical models and hydrodynamical simulations have suggested that stars could form within galactic outflows, representing a new mode of star-formation that differs significantly from the typical star formation in star forming discs. In this paper, we examine 12 local galaxies with powerful Active Galactic Nuclei and high star-formation rate using spectroscopic data from the X-shooter spectrograph at the Very Large Telescope. We investigate the excitation mechanism and physical properties of these outflows via spatially resolved diagnostic diagrams (along with tests to rule out contribution by shocks and external photoionisation). Out of the seven galaxies with clearly detected outflows, we find robust evidence for star formation within the outflow of one galaxy (IRAS 20551-4250), with two additional galaxies showing tentative signs (IRAS 13120-5453 and F13229-2934). Therefore, our findings support previous results that star formation inside outflows can be a relatively common phenomenon among these active galaxies and may have played an important role in the formation and evolution of the spheroidal component of galaxies. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2512_10924 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Signatures of star formation inside galactic outflows Ong, Dily Duan Yi D'Eugenio, Francesco Maiolino, Roberto Arribas, Santiago Belfiore, Francesco Bellocchi, Enrica Carniani, Stefano Cazzoli, Sara Cresci, Giovanni Fabian, Andrew Ishibashi, Wako Mannucci, Filippo Marconi, Alessandro Russell, Helen Sturm, Eckhard Venturi, Giacomo Astrophysics of Galaxies Instrumentation and Methods for Astrophysics Observations have suggested that galactic outflows contain substantial amounts of dense and clumpy molecular gas, creating favourable conditions for igniting star formation. Indeed, theoretical models and hydrodynamical simulations have suggested that stars could form within galactic outflows, representing a new mode of star-formation that differs significantly from the typical star formation in star forming discs. In this paper, we examine 12 local galaxies with powerful Active Galactic Nuclei and high star-formation rate using spectroscopic data from the X-shooter spectrograph at the Very Large Telescope. We investigate the excitation mechanism and physical properties of these outflows via spatially resolved diagnostic diagrams (along with tests to rule out contribution by shocks and external photoionisation). Out of the seven galaxies with clearly detected outflows, we find robust evidence for star formation within the outflow of one galaxy (IRAS 20551-4250), with two additional galaxies showing tentative signs (IRAS 13120-5453 and F13229-2934). Therefore, our findings support previous results that star formation inside outflows can be a relatively common phenomenon among these active galaxies and may have played an important role in the formation and evolution of the spheroidal component of galaxies. |
| title | Signatures of star formation inside galactic outflows |
| topic | Astrophysics of Galaxies Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2512.10924 |