Empirical SED Templates for Star Clusters Observed with HST and JWST: No Strong PAH or IR Dust Emission after 5 Myr
2025; IOP Publishing; Volume: 982; Issue: 1 Linguagem: Inglês
10.3847/1538-4357/adb3a2
ISSN1538-4357
AutoresBradley C. Whitmore, Rupali Chandar, Janice Lee, Kiana F. Henny, M. Jimena Rodríguez, Dalya Baron, Frank Bigiel, M. Boquien, Mélanie Chevance, Ryan Chown, Daniel A. Dale, Matthew Floyd, Kathryn Grasha, Simon C. O. Glover, Oleg Y. Gnedin, Hamid Hassani, R. Indebetouw, Anand Utsav Kapoor, Kirsten L. Larson, Adam K. Leroy, Daniel Maschmann, Fabian Scheuermann, Jessica Sutter, E. Schinnerer, Sumit K. Sarbadhicary, David A. Thilker, Thomas G. Williams, Aida Wofford,
Tópico(s)Galaxies: Formation, Evolution, Phenomena
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