JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M82 Galactic Wind

Alberto D. Bolatto; Rebecca C. Levy; Elizabeth Tarantino; Martha L. Boyer; Deanne B. Fisher; Serena A. Cronin; Adam K. Leroy; Ralf S. Klessen; J. D. Smith; Danielle A. Berg; Torsten Böker; Leindert A. Boogaard; Eve C. Ostriker; Todd A. Thompson; Juergen Ott; Laura Lenkić; Laura A. Lopez; Daniel A. Dale; Sylvain Veilleux; Paul P. van der Werf; Simon C.O. Glover; Karin M. Sandstrom; Evan D. Skillman; John Chisholm; Vicente Villanueva; Thomas S.Y. Lai; Sebastian Lopez; Elisabeth A.C. Mills; Kimberly L. Emig; Lee Armus; Divakara Mayya; David S. Meier; Ilse De Looze; Rodrigo Herrera-Camus; Fabian Walter; Mónica Relaño; Hannah B. Koziol; Joshua Marvil; María J. Jiménez-Donaire; Paul Martini

doi:10.3847/1538-4357/ad33c8

JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M82 Galactic Wind

Alberto D. Bolatto
, Rebecca C. Levy
, Elizabeth Tarantino
, Martha L. Boyer
, Deanne B. Fisher
, Serena A. Cronin
, Adam K. Leroy
, Ralf S. Klessen
, J. D. Smith
, Danielle A. Berg
, Torsten Böker
, Leindert A. Boogaard
, Eve C. Ostriker
, Todd A. Thompson
, Juergen Ott
, Laura Lenkić
, Laura A. Lopez
, Daniel A. Dale
, Sylvain Veilleux
, Paul P. van der Werf

Simon C.O. Glover, Karin M. Sandstrom, Evan D. Skillman, John Chisholm, Vicente Villanueva, Thomas S.Y. Lai, Sebastian Lopez, Elisabeth A.C. Mills, Kimberly L. Emig, Lee Armus, Divakara Mayya, David S. Meier, Ilse De Looze, Rodrigo Herrera-Camus, Fabian Walter, Mónica Relaño, Hannah B. Koziol, Joshua Marvil, María J. Jiménez-Donaire, Paul Martini

Research output: Contribution to journal › Article › peer-review

25 Scopus citations

Abstract

We present new observations of the central 1 kpc of the M82 starburst obtained with the James Webb Space Telescope near-infrared camera instrument at a resolution θ ∼ 0.″05-0.″1 (∼1-2 pc). The data comprises images in three mostly continuum filters (F140M, F250M, and F360M), and filters that contain [Fe ii] (F164N), H₂ v = 1 → 0 (F212N), and the 3.3 μm polycyclic aromatic hydrocarbon (PAH) feature (F335M). We find prominent plumes of PAH emission extending outward from the central starburst region, together with a network of complex filamentary substructures and edge-brightened bubble-like features. The structure of the PAH emission closely resembles that of the ionized gas, as revealed in Paschen α 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.

Original language	English (US)
Article number	63
Journal	Astrophysical Journal
Volume	967
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/ad33c8
State	Published - May 1 2024

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/1538-4357/ad33c8

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Bolatto, A. D., Levy, R. C., Tarantino, E., Boyer, M. L., Fisher, D. B., Cronin, S. A., Leroy, A. K., Klessen, R. S., Smith, J. D., Berg, D. A., Böker, T., Boogaard, L. A., Ostriker, E. C., Thompson, T. A., Ott, J., Lenkić, L., Lopez, L. A., Dale, D. A., Veilleux, S., ... Martini, P. (2024). JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M82 Galactic Wind. Astrophysical Journal, 967(1), Article 63. https://doi.org/10.3847/1538-4357/ad33c8

@article{f36e46b8133c4f6fa212121c76d7aba4,

title = "JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M82 Galactic Wind",

abstract = "We present new observations of the central 1 kpc of the M82 starburst obtained with the James Webb Space Telescope near-infrared camera instrument at a resolution θ ∼ 0.″05-0.″1 (∼1-2 pc). The data comprises images in three mostly continuum filters (F140M, F250M, and F360M), and filters that contain [Fe ii] (F164N), H2 v = 1 → 0 (F212N), and the 3.3 μm polycyclic aromatic hydrocarbon (PAH) feature (F335M). We find prominent plumes of PAH emission extending outward from the central starburst region, together with a network of complex filamentary substructures and edge-brightened bubble-like features. The structure of the PAH emission closely resembles that of the ionized gas, as revealed in Paschen α 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.",

author = "Bolatto, \{Alberto D.\} and Levy, \{Rebecca C.\} and Elizabeth Tarantino and Boyer, \{Martha L.\} and Fisher, \{Deanne B.\} and Cronin, \{Serena A.\} and Leroy, \{Adam K.\} and Klessen, \{Ralf S.\} and Smith, \{J. D.\} and Berg, \{Danielle A.\} and Torsten B{\"o}ker and Boogaard, \{Leindert A.\} and Ostriker, \{Eve C.\} and Thompson, \{Todd A.\} and Juergen Ott and Laura Lenki{\'c} and Lopez, \{Laura A.\} and Dale, \{Daniel A.\} and Sylvain Veilleux and \{van der Werf\}, \{Paul P.\} and Glover, \{Simon C.O.\} and Sandstrom, \{Karin M.\} and Skillman, \{Evan D.\} and John Chisholm and Vicente Villanueva and Lai, \{Thomas S.Y.\} and Sebastian Lopez and Mills, \{Elisabeth A.C.\} and Emig, \{Kimberly L.\} and Lee Armus and Divakara Mayya and Meier, \{David S.\} and \{De Looze\}, Ilse and Rodrigo Herrera-Camus and Fabian Walter and M{\'o}nica Rela{\~n}o and Koziol, \{Hannah B.\} and Joshua Marvil and Jim{\'e}nez-Donaire, \{Mar{\'i}a J.\} and Paul Martini",

note = "Publisher Copyright: {\textcopyright} 2024. The Author(s). Published by the American Astronomical Society.",

year = "2024",

month = may,

day = "1",

doi = "10.3847/1538-4357/ad33c8",

language = "English (US)",

volume = "967",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1",

}

Bolatto, AD, Levy, RC, Tarantino, E, Boyer, ML, Fisher, DB, Cronin, SA, Leroy, AK, Klessen, RS, Smith, JD, Berg, DA, Böker, T, Boogaard, LA, Ostriker, EC, Thompson, TA, Ott, J, Lenkić, L, Lopez, LA, Dale, DA, Veilleux, S, van der Werf, PP, Glover, SCO, Sandstrom, KM, Skillman, ED, Chisholm, J, Villanueva, V, Lai, TSY, Lopez, S, Mills, EAC, Emig, KL, Armus, L, Mayya, D, Meier, DS, De Looze, I, Herrera-Camus, R, Walter, F, Relaño, M, Koziol, HB, Marvil, J, Jiménez-Donaire, MJ & Martini, P 2024, 'JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M82 Galactic Wind', Astrophysical Journal, vol. 967, no. 1, 63. https://doi.org/10.3847/1538-4357/ad33c8

TY - JOUR

T1 - JWST Observations of Starbursts

T2 - Polycyclic Aromatic Hydrocarbon Emission at the Base of the M82 Galactic Wind

AU - Bolatto, Alberto D.

AU - Levy, Rebecca C.

AU - Tarantino, Elizabeth

AU - Boyer, Martha L.

AU - Fisher, Deanne B.

AU - Cronin, Serena A.

AU - Leroy, Adam K.

AU - Klessen, Ralf S.

AU - Smith, J. D.

AU - Berg, Danielle A.

AU - Böker, Torsten

AU - Boogaard, Leindert A.

AU - Ostriker, Eve C.

AU - Thompson, Todd A.

AU - Ott, Juergen

AU - Lenkić, Laura

AU - Lopez, Laura A.

AU - Dale, Daniel A.

AU - Veilleux, Sylvain

AU - van der Werf, Paul P.

AU - Glover, Simon C.O.

AU - Sandstrom, Karin M.

AU - Skillman, Evan D.

AU - Chisholm, John

AU - Villanueva, Vicente

AU - Lai, Thomas S.Y.

AU - Lopez, Sebastian

AU - Mills, Elisabeth A.C.

AU - Emig, Kimberly L.

AU - Armus, Lee

AU - Mayya, Divakara

AU - Meier, David S.

AU - De Looze, Ilse

AU - Herrera-Camus, Rodrigo

AU - Walter, Fabian

AU - Relaño, Mónica

AU - Koziol, Hannah B.

AU - Marvil, Joshua

AU - Jiménez-Donaire, María J.

AU - Martini, Paul

PY - 2024/5/1

Y1 - 2024/5/1

N2 - We present new observations of the central 1 kpc of the M82 starburst obtained with the James Webb Space Telescope near-infrared camera instrument at a resolution θ ∼ 0.″05-0.″1 (∼1-2 pc). The data comprises images in three mostly continuum filters (F140M, F250M, and F360M), and filters that contain [Fe ii] (F164N), H2 v = 1 → 0 (F212N), and the 3.3 μm polycyclic aromatic hydrocarbon (PAH) feature (F335M). We find prominent plumes of PAH emission extending outward from the central starburst region, together with a network of complex filamentary substructures and edge-brightened bubble-like features. The structure of the PAH emission closely resembles that of the ionized gas, as revealed in Paschen α 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.

AB - We present new observations of the central 1 kpc of the M82 starburst obtained with the James Webb Space Telescope near-infrared camera instrument at a resolution θ ∼ 0.″05-0.″1 (∼1-2 pc). The data comprises images in three mostly continuum filters (F140M, F250M, and F360M), and filters that contain [Fe ii] (F164N), H2 v = 1 → 0 (F212N), and the 3.3 μm polycyclic aromatic hydrocarbon (PAH) feature (F335M). We find prominent plumes of PAH emission extending outward from the central starburst region, together with a network of complex filamentary substructures and edge-brightened bubble-like features. The structure of the PAH emission closely resembles that of the ionized gas, as revealed in Paschen α 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.

UR - https://www.scopus.com/pages/publications/85193614228

UR - https://www.scopus.com/pages/publications/85193614228#tab=citedBy

U2 - 10.3847/1538-4357/ad33c8

DO - 10.3847/1538-4357/ad33c8

M3 - Article

AN - SCOPUS:85193614228

SN - 0004-637X

VL - 967

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 63

ER -

JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M82 Galactic Wind

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