JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M 82 Galactic Wind
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2024
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| author | Bolatto, Alberto D. Levy, Rebecca C. Tarantino, Elizabeth Boyer, Martha L. Fisher, Deanne B. Leroy, Adam K. Cronin, Serena A. Klessen, Ralf S. Smith, J. D. Berg, Dannielle A. Boeker, Torsten Boogaard, Leindert A. Ostriker, Eve C. Thompson, Todd A. Ott, Juergen Lenkic, Laura Lopez, Laura A. Dale, Daniel A. Veilleux, Sylvain van der Werf, Paul P. Glover, Simon C. O. Sandstrom, Karin M. Skillman, Evan D. Chisholm, John Villanueva, Vicente Lai, Thomas S. -Y. Lopez, Sebastian Mills, Elisabeth A. C. Emig, Kimberly L. Armus, Lee Maya, Divakara Meier, David S. De Looze, Ilse Herrera-Camus, Rodrigo Walter, Fabian Relano, Monica Koziol, Hannah B. Marvil, Joshua Jimenez-Donaire, Maria J. Martini, Paul |
| author_facet | Bolatto, Alberto D. Levy, Rebecca C. Tarantino, Elizabeth Boyer, Martha L. Fisher, Deanne B. Leroy, Adam K. Cronin, Serena A. Klessen, Ralf S. Smith, J. D. Berg, Dannielle A. Boeker, Torsten Boogaard, Leindert A. Ostriker, Eve C. Thompson, Todd A. Ott, Juergen Lenkic, Laura Lopez, Laura A. Dale, Daniel A. Veilleux, Sylvain van der Werf, Paul P. Glover, Simon C. O. Sandstrom, Karin M. Skillman, Evan D. Chisholm, John Villanueva, Vicente Lai, Thomas S. -Y. Lopez, Sebastian Mills, Elisabeth A. C. Emig, Kimberly L. Armus, Lee Maya, Divakara Meier, David S. De Looze, Ilse Herrera-Camus, Rodrigo Walter, Fabian Relano, Monica Koziol, Hannah B. Marvil, Joshua Jimenez-Donaire, Maria J. Martini, Paul |
| contents | We present new observations of the central 1 kpc of the M 82 starburst obtained with the James Webb Space Telescope (JWST) near-infrared camera (NIRCam) instrument at a resolution ~0.05"-0.1" (~1-2 pc). The data comprises images in three mostly continuum filters (F140M, F250M, and F360M), and filters that contain [FeII] (F164N), H2 v=1-0 (F212N), and the 3.3 um PAH feature (F335M). We find prominent plumes of PAH emission extending outward from the central starburst region, together with a network of complex filamentary substructure and edge-brightened bubble-like features. The structure of the PAH emission closely resembles that of the ionized gas, as revealed in Paschen alpha and free-free radio emission. We discuss the origin of the structure, and suggest the PAHs are embedded in a combination of neutral, molecular, and photoionized gas. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2401_16648 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M 82 Galactic Wind Bolatto, Alberto D. Levy, Rebecca C. Tarantino, Elizabeth Boyer, Martha L. Fisher, Deanne B. Leroy, Adam K. Cronin, Serena A. Klessen, Ralf S. Smith, J. D. Berg, Dannielle A. Boeker, Torsten Boogaard, Leindert A. Ostriker, Eve C. Thompson, Todd A. Ott, Juergen Lenkic, Laura Lopez, Laura A. Dale, Daniel A. Veilleux, Sylvain van der Werf, Paul P. Glover, Simon C. O. Sandstrom, Karin M. Skillman, Evan D. Chisholm, John Villanueva, Vicente Lai, Thomas S. -Y. Lopez, Sebastian Mills, Elisabeth A. C. Emig, Kimberly L. Armus, Lee Maya, Divakara Meier, David S. De Looze, Ilse Herrera-Camus, Rodrigo Walter, Fabian Relano, Monica Koziol, Hannah B. Marvil, Joshua Jimenez-Donaire, Maria J. Martini, Paul Astrophysics of Galaxies We present new observations of the central 1 kpc of the M 82 starburst obtained with the James Webb Space Telescope (JWST) near-infrared camera (NIRCam) instrument at a resolution ~0.05"-0.1" (~1-2 pc). The data comprises images in three mostly continuum filters (F140M, F250M, and F360M), and filters that contain [FeII] (F164N), H2 v=1-0 (F212N), and the 3.3 um PAH feature (F335M). We find prominent plumes of PAH emission extending outward from the central starburst region, together with a network of complex filamentary substructure and edge-brightened bubble-like features. The structure of the PAH emission closely resembles that of the ionized gas, as revealed in Paschen alpha and free-free radio emission. We discuss the origin of the structure, and suggest the PAHs are embedded in a combination of neutral, molecular, and photoionized gas. |
| title | JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M 82 Galactic Wind |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2401.16648 |