JWST Observations of Starbursts: Massive Star Clusters in the Central Starburst of M82

We present a near infrared (NIR) candidate star cluster catalog for the central kiloparsec of M82 based on new JWST NIRCam images. We identify star cluster candidates using the F250M filter, finding 1357 star cluster candidates with stellar masses \(>10^4\) M\(_\odot\). Compared to previous optic...

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Hauptverfasser: Levy, Rebecca C, Bolatto, Alberto D, Divakara Mayya, Cuevas-Otahola, Bolivia, Tarantino, Elizabeth, Boyer, Martha L, Boogaard, Leindert A, Böker, Torsten, Cronin, Serena A, Dale, Daniel A, Keaton Donaghue, Emig, Kimberly L, Fisher, Deanne B, Glover, Simon C O, Herrera-Camus, Rodrigo, Jiménez-Donaire, María J, Klessen, Ralf S, Lenkić, Laura, Leroy, Adam K, De Looze, Ilse, Meier, David S, Mills, Elisabeth A C, Ott, Juergen, Relaño, Mónica, Veilleux, Sylvain, Villanueva, Vicente, Fabian, Walter, Paul P van der Werf
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creator Levy, Rebecca C
Bolatto, Alberto D
Divakara Mayya
Cuevas-Otahola, Bolivia
Tarantino, Elizabeth
Boyer, Martha L
Boogaard, Leindert A
Böker, Torsten
Cronin, Serena A
Dale, Daniel A
Keaton Donaghue
Emig, Kimberly L
Fisher, Deanne B
Glover, Simon C O
Herrera-Camus, Rodrigo
Jiménez-Donaire, María J
Klessen, Ralf S
Lenkić, Laura
Leroy, Adam K
De Looze, Ilse
Meier, David S
Mills, Elisabeth A C
Ott, Juergen
Relaño, Mónica
Veilleux, Sylvain
Villanueva, Vicente
Fabian, Walter
Paul P van der Werf
description We present a near infrared (NIR) candidate star cluster catalog for the central kiloparsec of M82 based on new JWST NIRCam images. We identify star cluster candidates using the F250M filter, finding 1357 star cluster candidates with stellar masses \(>10^4\) M\(_\odot\). Compared to previous optical catalogs, nearly all (87%) of the candidates we identify are new. The star cluster candidates have a median intrinsic cluster radius of \(\approx\)1 pc and have stellar masses up to \(10^6\) M\(_\odot\). By comparing the color-color diagram to dust-free yggdrasil stellar population models, we estimate that the star cluster candidates have A\(_{\rm V}\sim3-24\) mag, corresponding to A\(_{\rm 2.5\mu m}\sim0.3-2.1\) mag. There is still appreciable dust extinction towards these clusters into the NIR. We measure the stellar masses of the star cluster candidates, assuming ages of 0 and 8 Myr. The slope of the resulting cluster mass function is \(\beta=1.9\pm0.2\), in excellent agreement with studies of star clusters in other galaxies.
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subjects Astronomical models
Candidates
Color-color diagram
Cosmic dust
Galactic clusters
Galaxies
Image filters
Infrared imagery
Infrared stars
James Webb Space Telescope
Massive stars
Near infrared radiation
Star clusters
Stellar age
title JWST Observations of Starbursts: Massive Star Clusters in the Central Starburst of M82
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