2603.12200
2026-06-19
astro-ph.GA
版本更新
50%
GATOS XIV: The first direct kinematic evidence of dusty outflows from AGN via PAH kinematics of local Seyfert galaxies with JWST
GATOS XIV: 利用JWST对本地塞弗特星系的PAH运动学首次直接证明AGN尘埃外流的运动学证据
Fergus R. Donnan, Ismael García-Bernete, Dimitra Rigopoulou, Almudena Alonso-Herrero, Anelise Audibert, Enrica Bellocchi, Andrew Bunker, Steph Campbell, Françoise Combes, Richard Davies, Tanio Díaz-Santos, Juan A. Fernández-Ontiveros, Poshak Gandhi, Santiago García-Burillo, Omaria González-Martín, Erin K. S. Hicks, Laura Hermosa Muñoz, Sebastian F. Hoenig, Masatoshi Imanishi, Alvaro Labiano, Nancy A. Levenson, Miguel Pereira-Santaella, Cristina Ramos Almeida, Claudio Ricci, Rogemar A. Riffel, Daniel Rouan, David Rosario, Karin Sandstrom, Taro T. Shimizu, Marko Stalevski, Niranjan Thatte, Oscar Veenema, Lulu Zhang
专题命中
其他LLM
:prompting(abstract)
AI总结
利用JWST的NIRSpec IFU和MIRI MRS数据,通过PCA层析成像提取10个本地塞弗特星系中多环芳烃(PAH)的运动学,首次直接证明活动星系核(AGN)外流中存在尘埃,发现外流中的PAH更中性且更大。