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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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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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. 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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.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
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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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