2605.26864
2026-05-27
astro-ph.GA
Survival of very small carbonaceous dust grains in the inner-CGM of NGC 891 from JWST/MIRI MRS
来自JWST/MIRI MRS的NGC 891内CGM中极小微碳质尘埃的存活
Jérémy Chastenet, Ilse De Looze, Karl D. Gordon, Suzanne C. Madden, Monica Relaño, Karin M. Sandstrom, Dries Van De Putte, Maarten Baes, Simone Bianchi, Alberto D. Bolatto, Viviana Casasola, Daniel A. Dale, Sara Duval, Jacopo Fritz, Frédéric Galliano, Simon C. O. Glover, Stavroula Katsioli, Vasileios Katsis, Florian Kirchschlager, Ralf S. Klessen, Rebecca C. Levy, Sharon E. Meidt, Aleksandr V. Mosenkov, Kentaro Nagamine, Lara Pantoni, Helena M. Richie, Stefanie Walch, Thomas G. Williams, Emanuele M. Xilouris
AI总结
利用JWST/MIRI MRS观测NGC 891内周介质(CGM)的四个位置,通过PAHFIT模型分析中红外光谱,发现多环芳烃(PAHs)主导了先前报告的中红外发射,证明了PAHs在内CGM中的存活,并揭示了PAH特性随辐射场硬度的变化以及H2与PAH的紧密相关性。