JWST Observations of Starbursts: Relations between PAH features and CO clouds in the starburst galaxy M 82 (Corrigendum)

¹ Departamento de Astronomía, Universidad de Concepción, Barrio Universitario, Concepción, Chile
² Department of Astronomy, University of Maryland, College Park, MD 20742, USA
³ Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
⁴ Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia
⁵ ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)
⁶ Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA
⁷ IPAC, California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125, USA
⁸ Department of Physics & Astronomy, University of Wyoming, Laramie, WY 82071, USA
⁹ Sterrenkundig Observatorium, Ghent University, Krijgslaan 281 – S9, B9000 Ghent, Belgium
¹⁰ Departamento Física Teórica y del Cosmos, Universidad de Granada, E-18071 Granada, Spain
¹¹ Instituto Universitario Carlos I de Física Teórica y Computacional, Universidad de Granada, E-18071 Granada, Spain
¹² European Space Agency, c/o STScI, 3700 San Martin Drive, Baltimore, MD 21218, USA
¹³ Leiden Observatory, Leiden University, P.O. Box 9513 2300 RA, Leiden, The Netherlands
¹⁴ National Radio Astronomy Observatory, P.O. Box O 1003 Lopezville Road, Socorro, NM 87801, USA
¹⁵ New Mexico Institute of Mining and Technology, 801 Leroy Place, Socorro, NM 87801, USA
¹⁶ IPAC, California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125, USA
¹⁷ National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA
¹⁸ Millenium Nucleus for Galaxies (MINGAL), Chile
¹⁹ Ritter Astrophysical Research Center, University of Toledo, Toledo, OH 43606, USA
²⁰ Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
²¹ Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany

^⋆⋆ Corresponding author: vvillanueva@astro-udec.cl

This article has no abstract.