A PAH deficit in the starburst core of a distant spiral galaxy
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2025
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| author | Liu, Zhaoxuan Silverman, John D. Daddi, Emanuele Kalita, Boris S. Puglisi, Annagrazia Fei, Qinyue Renzini, Alvio Kashino, Daichi Valentino, Francesco Kartaltepe, Jeyhan S. Liu, Daizhong Pérez-González, Pablo G. McKinney, Jed Casey, Caitlin M. Ding, Xuheng Faisst, Andreas Franco, Maximilien Kakkad, Darshan Koekemoer, Anton M. Lambrides, Erini Gillman, Steven Gozaliasl, Ghassem McCracken, Henry Joy Rhodes, Jason Robertson, Brant E. Rodighiero, Giulia Rujopakarn, Wiphu Suzuki, Tomoko L. Tanaka, Takumi S. Vanderhoof, Brittany N. Vijayan, Aswin P. Cooper, Olivia R. Kaminsky, Aidan Magdis, Georgios E. Roy, Namrata |
| author_facet | Liu, Zhaoxuan Silverman, John D. Daddi, Emanuele Kalita, Boris S. Puglisi, Annagrazia Fei, Qinyue Renzini, Alvio Kashino, Daichi Valentino, Francesco Kartaltepe, Jeyhan S. Liu, Daizhong Pérez-González, Pablo G. McKinney, Jed Casey, Caitlin M. Ding, Xuheng Faisst, Andreas Franco, Maximilien Kakkad, Darshan Koekemoer, Anton M. Lambrides, Erini Gillman, Steven Gozaliasl, Ghassem McCracken, Henry Joy Rhodes, Jason Robertson, Brant E. Rodighiero, Giulia Rujopakarn, Wiphu Suzuki, Tomoko L. Tanaka, Takumi S. Vanderhoof, Brittany N. Vijayan, Aswin P. Cooper, Olivia R. Kaminsky, Aidan Magdis, Georgios E. Roy, Namrata |
| contents | We present high-resolution and spatially-matched observations with JWST and ALMA of a starburst galaxy (PACS-830) at $z=1.46$. The NIRCam observations mainly trace the stellar light while the CO ($J$=5--4) observations map the dense molecular gas at kpc scales. Both datasets reveal the morphology to be that of a gas/dust rich bulge with two extending arms, together resembling a grand-design spiral galaxy. The more pronounced arm contributes 21 $\pm$ 6\% of the total CO emission. These results demonstrate that starburst activity at high redshift can be triggered, without undergoing a highly disruptive major merger. We assess the strength and distribution of star formation using two tracers: (1) Polycyclic Aromatic Hydrocarbons (PAHs) emission detected at $8~μ$m ($L_8$) with a MIRI/F1800W image, and (2) $L_\mathrm{IR}$, inferred from the CO ($J$=5--4) map. The spatial profiles of the $L_\mathrm{IR}$ and $L_8$ are dissimilar, thus leading to a significant deficit of mid-IR ($L_8$) emission in the nucleus. We hypothesize that this is due to the destruction of PAH molecules by the intense ionizing radiation field or decreased emission in the photodissociation region, as seen in nearby star-forming regions and consistent with the galaxy-wide properties of distant starbursts. This study reveals spatial variations in the $L_8$ to $L_\mathrm{IR}$ ratio for the first time at $z>1$, in agreement with expectations from theory. Our analysis underscores the pivotal role of joint high-resolution observations with JWST and ALMA in discerning the different phases of the interstellar medium (ISM) and revealing internal physics in galaxy substructures. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_09728 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | A PAH deficit in the starburst core of a distant spiral galaxy Liu, Zhaoxuan Silverman, John D. Daddi, Emanuele Kalita, Boris S. Puglisi, Annagrazia Fei, Qinyue Renzini, Alvio Kashino, Daichi Valentino, Francesco Kartaltepe, Jeyhan S. Liu, Daizhong Pérez-González, Pablo G. McKinney, Jed Casey, Caitlin M. Ding, Xuheng Faisst, Andreas Franco, Maximilien Kakkad, Darshan Koekemoer, Anton M. Lambrides, Erini Gillman, Steven Gozaliasl, Ghassem McCracken, Henry Joy Rhodes, Jason Robertson, Brant E. Rodighiero, Giulia Rujopakarn, Wiphu Suzuki, Tomoko L. Tanaka, Takumi S. Vanderhoof, Brittany N. Vijayan, Aswin P. Cooper, Olivia R. Kaminsky, Aidan Magdis, Georgios E. Roy, Namrata Astrophysics of Galaxies We present high-resolution and spatially-matched observations with JWST and ALMA of a starburst galaxy (PACS-830) at $z=1.46$. The NIRCam observations mainly trace the stellar light while the CO ($J$=5--4) observations map the dense molecular gas at kpc scales. Both datasets reveal the morphology to be that of a gas/dust rich bulge with two extending arms, together resembling a grand-design spiral galaxy. The more pronounced arm contributes 21 $\pm$ 6\% of the total CO emission. These results demonstrate that starburst activity at high redshift can be triggered, without undergoing a highly disruptive major merger. We assess the strength and distribution of star formation using two tracers: (1) Polycyclic Aromatic Hydrocarbons (PAHs) emission detected at $8~μ$m ($L_8$) with a MIRI/F1800W image, and (2) $L_\mathrm{IR}$, inferred from the CO ($J$=5--4) map. The spatial profiles of the $L_\mathrm{IR}$ and $L_8$ are dissimilar, thus leading to a significant deficit of mid-IR ($L_8$) emission in the nucleus. We hypothesize that this is due to the destruction of PAH molecules by the intense ionizing radiation field or decreased emission in the photodissociation region, as seen in nearby star-forming regions and consistent with the galaxy-wide properties of distant starbursts. This study reveals spatial variations in the $L_8$ to $L_\mathrm{IR}$ ratio for the first time at $z>1$, in agreement with expectations from theory. Our analysis underscores the pivotal role of joint high-resolution observations with JWST and ALMA in discerning the different phases of the interstellar medium (ISM) and revealing internal physics in galaxy substructures. |
| title | A PAH deficit in the starburst core of a distant spiral galaxy |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2505.09728 |