A bright inner disk and structures in the transition disk around the very low-mass star CIDA 1

The frequency of Earth-sized planets in habitable zones appears to be higher around M-dwarfs, making these systems exciting laboratories to investigate planet formation. Observations of protoplanetary disks around very low-mass stars and brown dwarfs remain challenging and little is known about thei...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-05, Vol.649, p.A122
Hauptverfasser:	Pinilla, P., Kurtovic, N. T., Benisty, M., Manara, C. F., Natta, A., Sanchis, E., Tazzari, M., Stammler, S. M., Ricci, L., Testi, L.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astrophysics Deposition Dust Extrasolar planets Low mass stars Morphology Planet formation Planetary evolution Protoplanetary disks Radiative transfer Sciences of the Universe
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