The Potential of the SPHEREx Mission for Characterizing Polycyclic Aromatic Hydrocarbon 3.3 μm Emission in Nearby Galaxies

Together with gas, stars, and supermassive black holes, dust is crucial in stellar and galaxy evolution. Hence, understanding galaxies’ dust properties across cosmic time is critical to studying their evolution. In addition to photometric constraints on the absorption of blue light and its reemissio...

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Detalhes bibliográficos

Principais autores:	Edward Zhang, Andreas L. Faisst, Brendan P. Crill, Hanae Inami, Thomas Lai, Youichi Ohyama, Jeonghyun Pyo, Rachel Akeson, Matthew L. N. Ashby, James J. Bock, Yun-Ting Cheng, Yi-Kuan Chiang, Asantha Cooray, Olivier Doré, Richard M. Feder, Yongjung Kim, Bomee Lee, Daniel Masters, Gary Melnick, Roberta Paladini, Michael W. Werner
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
coleção:	The Astrophysical Journal
Assuntos:	Interstellar medium Polycyclic aromatic hydrocarbons Dust composition Telescopes Galaxy spectroscopy
Acesso em linha:	https://doi.org/10.3847/1538-4357/adfd5a
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