The PHANGS-JWST Treasury survey: star formation, feedback, and dust physics at high angular resolution in nearby galaxies

Janice C. Lee*, Karin M. Sandstrom, Adam K. Leroy, David A. Thilker, Eva Schinnerer, Erik Rosolowsky, Kirsten L. Larson, Oleg V. Egorov, Thomas G. Williams, Judy Schmidt, Eric Emsellem, Gagandeep S. Anand, Ashley T. Barnes, Francesco Belfiore, Ivana Beslic, Frank Bigiel, Guillermo A. Blanc, Alberto D. Bolatto, Mederic Boquien, Jakob den BrokYixian Cao, Rupali Chandar, Jeremy Chastenet, Melanie Chevance, I-Da Chiang, Enrico Congiu, Daniel A. Dale, Sinan Deger, Cosima Eibensteiner, Christopher M. Faesi, Simon C. O. Glover, Kathryn Grasha, Brent Groves, Hamid Hassani, Kiana F. Henny, Jonathan D. Henshaw, Nils Hoyer, Annie Hughes, Sarah Jeffreson, Marıa J. Jimenez-Donaire, Jaeyeon Kim, Hwihyun Kim, Ralf S. Klessen, Eric W. Koch, Kathryn Kreckel, J. M. Diederik Kruijssen, Jing Li, Daizhong Liu, Laura A. Lopez, Daniel Maschmann, Ness Mayker Chen, Sharon E. Meidt, Eric J. Murphy, Justus Neumann, Nadine Neumayer, Hsi-An Pan, Ismael Pessa, Jerome Pety, Miguel Querejeta, Francesca Pinna, M. Jimena Rodrıguez, Toshiki Saito, Patricia Sanchez-Blazquez, Francesco Santoro, Amy Sardone, Rowan J. Smith, Mattia C. Sormani, Fabian Scheuermann, Sophia K. Stuber, Jessica Sutter, Jiayi Sun, Yu-Hsuan Teng, Robin G. Tress, Antonio Usero, Elizabeth J. Watkins, Bradley C. Whitmore, Alessandro Razza

*Corresponding author for this work

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

Fingerprint

Dive into the research topics of 'The PHANGS-JWST Treasury survey: star formation, feedback, and dust physics at high angular resolution in nearby galaxies'. Together they form a unique fingerprint.

Physics