FEAST: a NIRSpec/MOS survey of emerging young star clusters in NGC 628
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| Format: | Preprint |
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2026
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| _version_ | 1866918381631832064 |
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| author | Vieira, Helena Faustino Adamo, Angela Shane, Neville Smith, Linda J. Bik, Arjan Lai, Thomas S. -Y. Pedrini, Alex Hunt, Leslie K. Linden, Sean T. Bortolini, Giacomo Buckner, Anne S. Calzetti, Daniela Correnti, Matteo Duarte-Cabral, Ana Grasha, Kathryn Johnson, Kelsey E. Lapeer, Drew Messa, Matteo Östlin, Göran Roos, Linn Sabbi, Elena |
| author_facet | Vieira, Helena Faustino Adamo, Angela Shane, Neville Smith, Linda J. Bik, Arjan Lai, Thomas S. -Y. Pedrini, Alex Hunt, Leslie K. Linden, Sean T. Bortolini, Giacomo Buckner, Anne S. Calzetti, Daniela Correnti, Matteo Duarte-Cabral, Ana Grasha, Kathryn Johnson, Kelsey E. Lapeer, Drew Messa, Matteo Östlin, Göran Roos, Linn Sabbi, Elena |
| contents | JWST can pierce through dusty molecular clouds to study the early stages of star formation, where young star clusters are actively driving stellar feedback and still emerging from their natal cloud. We present a first look of the JWST/NIRSpec multiplex spectroscopy observations acquired by the Feedback in Emerging extrAgalactic Star clusTers (FEAST) program for the nearby spiral galaxy NGC628. We showcase JWST's ability to resolve the spectral properties of emerging young star clusters (eYSCs) and their immediate interstellar medium (ISM) by focusing on a bright star-forming complex ($0.5\times0.5~\mathrm{kpc}^2$) in the northern spiral arm as a science proof-of-concept. The eYSC spectra are rich in ionized gas (from HII regions), as well as warm H$_2$ and polycyclic aromatic hydrocarbon (PAH) emission from photodissociation regions (PDRs), consistent with young star formation. $\mathrm{Pa}α$ equivalent widths and H/He ionizing photon fluxes both indicate the presence of hot, young massive stars (O8.5V-O8V), consistent with photometry SED estimates. The ionized gas is highly correlated with H$_2$ and PAH emission, suggesting that the PDR morphology evolves as clusters emerge from their natal cloud. We find a photoionization-dominated regime from independent line diagnostics, with little contribution from Supernovae-driven shocks, highlighting the importance of pre-Supernovae feedback when massive stars are present. This pilot study showcases how JWST's multiplex spectroscopy mode can disentangle the mechanisms present in the youngest stages of star formation for the first time outside the Local Group. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2603_09866 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | FEAST: a NIRSpec/MOS survey of emerging young star clusters in NGC 628 Vieira, Helena Faustino Adamo, Angela Shane, Neville Smith, Linda J. Bik, Arjan Lai, Thomas S. -Y. Pedrini, Alex Hunt, Leslie K. Linden, Sean T. Bortolini, Giacomo Buckner, Anne S. Calzetti, Daniela Correnti, Matteo Duarte-Cabral, Ana Grasha, Kathryn Johnson, Kelsey E. Lapeer, Drew Messa, Matteo Östlin, Göran Roos, Linn Sabbi, Elena Astrophysics of Galaxies JWST can pierce through dusty molecular clouds to study the early stages of star formation, where young star clusters are actively driving stellar feedback and still emerging from their natal cloud. We present a first look of the JWST/NIRSpec multiplex spectroscopy observations acquired by the Feedback in Emerging extrAgalactic Star clusTers (FEAST) program for the nearby spiral galaxy NGC628. We showcase JWST's ability to resolve the spectral properties of emerging young star clusters (eYSCs) and their immediate interstellar medium (ISM) by focusing on a bright star-forming complex ($0.5\times0.5~\mathrm{kpc}^2$) in the northern spiral arm as a science proof-of-concept. The eYSC spectra are rich in ionized gas (from HII regions), as well as warm H$_2$ and polycyclic aromatic hydrocarbon (PAH) emission from photodissociation regions (PDRs), consistent with young star formation. $\mathrm{Pa}α$ equivalent widths and H/He ionizing photon fluxes both indicate the presence of hot, young massive stars (O8.5V-O8V), consistent with photometry SED estimates. The ionized gas is highly correlated with H$_2$ and PAH emission, suggesting that the PDR morphology evolves as clusters emerge from their natal cloud. We find a photoionization-dominated regime from independent line diagnostics, with little contribution from Supernovae-driven shocks, highlighting the importance of pre-Supernovae feedback when massive stars are present. This pilot study showcases how JWST's multiplex spectroscopy mode can disentangle the mechanisms present in the youngest stages of star formation for the first time outside the Local Group. |
| title | FEAST: a NIRSpec/MOS survey of emerging young star clusters in NGC 628 |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2603.09866 |