MIRI MRS Observations of Beta Pictoris. II. The Spectroscopic Case for a Recent Giant Collision

Modeling observations of the archetypal debris disk around β Pic, obtained in 2023 January with the MIRI Medium Resolution Spectrograph on board JWST, reveals significant differences compared with that obtained with the Infrared Spectrograph on board Spitzer. The bright 5–15 μ m continuum excess mod...

Täydet tiedot

Bibliografiset tiedot

Päätekijät:	Christine H. Chen, Cicero X. Lu, Kadin Worthen, David R. Law, B. A. Sargent, Amaya Moro-Martin, G. C. Sloan, Carey M. Lisse, Dan M. Watson, Julien H. Girard, Yiwei Chai, Dean C. Hines, Jens Kammerer, Alexis Li, Marshall Perrin, Laurent Pueyo, Isabel Rebollido, Karl R. Stapelfeldt, Christopher Stark, Michael W. Werner
Aineistotyyppi:	Artigo
Kieli:	Inglês
Julkaistu:	IOP Publishing 2024-01-01
Sarja:	The Astrophysical Journal
Aiheet:	Debris disks Infrared astronomy Planetary system formation
Linkit:	https://doi.org/10.3847/1538-4357/ad60bb
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