_version_ 1866910416705159168
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