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Polycyclic aromatic hydrocarbons (PAHs) are responsible for strong mid-IR emission features near star-forming regions. It is well known that low-metallicity environments exhibit weaker PAH emission, but it is not clear how the metallicity affects the
Externí odkaz:
http://arxiv.org/abs/2410.18909
Autor:
Coyle, Laura E., Matsuura, Shuji, Perrin, Marshall D., Rowe, Jason F., Metchev, Stanimir, Hoffman, Kelsey L., Lavigne, Jean-François, Montembeault, Yan, Hales, Joelene, Lambier, Samantha, Lizotte, Déreck, Miles-Páez, Paulo, Sikora, James, Suárez, Genaro, Swidinsky, Nicholas
Publikováno v:
Proceedings of SPIE; August 2022, Vol. 12180 Issue: 1 p121800A-121800A-10, 12058211p
Autor:
Rowe, Jason F., Metchev, Stanimir, Hoffman, Kelsey L., Lavigne, Jean-François, Montembeault, Yan, Hales, Joelene, Lambier, Samantha, Lizotte, Déreck, Miles-Páez, Paulo, Sikora, James, Suárez, Genaro, Swidinsky, Nicholas
Publikováno v:
Proceedings of SPIE; 5/28/2022, Vol. 12180, p121800A-121800A-10, 1p