Shockingly Bright Warm Carbon Monoxide Molecular Features in the Supernova Remnant Cassiopeia A Revealed by JWST

Shockingly Bright Warm Carbon Monoxide Molecular Features in the Supernova Remnant Cassiopeia A Revealed by JWST

We present JWST NIRCam (F356W and F444W filters) and MIRI (F770W) images and NIRSpec Integral Field Unit (IFU) spectroscopy of the young Galactic supernova remnant Cassiopeia A (Cas A) to probe the physical conditions for molecular CO formation and destruction in supernova ejecta. We obtained the da...

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Xehetasun bibliografikoak
Egile Nagusiak: Rho, J, Park, S, Arendt, R, Matsuura, M, Milisavljevic, D, Temim, T, De Looze, I, Blair, WP, Rest, A, Fox, O, Ravi, AP, Koo, B, Barlow, M, Burrows, A, Chevalier, R, Clayton, G, Fesen, R, Fransson, C, Fryer, C, Gomez, HL, Janka, H, Kirchschlager, F, Laming, JM, Orlando, S, Posselt, B
Formatua: Journal article
Hizkuntza:English
Argitaratua: American Astronomical Society 2024

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