JWST/NIRCam Detection of the Fomalhaut C Debris Disk in Scattered Light

Observations of debris disks offer important insights into the formation and evolution of planetary systems. Though M dwarfs make up approximately 80% of nearby stars, very few M dwarf debris disks have been studied in detail—making it unclear how or if the information gleaned from studying debris d...

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Veröffentlicht in:	Astrophysical journal. Letters 2024-05, Vol.967 (1), p.L8
Hauptverfasser:	Lawson, Kellen, Schlieder, Joshua E., Leisenring, Jarron M., Bogat, Ell, Beichman, Charles A., Bryden, Geoffrey, Gáspár, András, Groff, Tyler D., McElwain, Michael W., Meyer, Michael R., Barclay, Thomas, Calissendorff, Per, De Furio, Matthew, Li, Yiting, Rieke, Marcia J., Ygouf, Marie, Greene, Thomas P., Girard, Julien H., Gennaro, Mario, Kammerer, Jens, Rest, Armin, Roellig, Thomas L., Sunnquist, Ben
Format:	Artikel
Sprache:	eng
Schlagworte:	Coronagraphic imaging Debris Debris disks Detritus Direct imaging Disks High contrast techniques Infrared cameras James Webb Space Telescope Light M dwarf stars Massive stars Planetary evolution Planetary systems Radio telescopes Red dwarf stars Stars
Online-Zugang:	Volltext
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