SPHERE H-band observations resolve a smaller, thicker, brighter disk with inner spirals around V721 CrA and a larger disk with a dark lane around BN CrA, both consistent with their locations in the CrA star-forming region.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.SR 3verdicts
UNVERDICTED 3representative citing papers
JH 223 shows a 250 G dipolar magnetic field truncating its disk near corotation, with accretion columns warping the inner disk to produce 3.31-day periodic dips in brightness.
Radial velocity measurements from NIR spectra show one TWA candidate as a spectroscopic binary with 41.9% membership probability and the other as a likely single member with 99.5% probability.
citing papers explorer
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Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): V721 CrA and BN CrA have wide and structured disks in polarised IR
SPHERE H-band observations resolve a smaller, thicker, brighter disk with inner spirals around V721 CrA and a larger disk with a dark lane around BN CrA, both consistent with their locations in the CrA star-forming region.
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The circumstellar environment of the young, low-mass dipper star JH 223. Accretion and large-scale magnetic field topology
JH 223 shows a 250 G dipolar magnetic field truncating its disk near corotation, with accretion columns warping the inner disk to produce 3.31-day periodic dips in brightness.
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Radial Velocities of Low-mass Candidate TWA Members
Radial velocity measurements from NIR spectra show one TWA candidate as a spectroscopic binary with 41.9% membership probability and the other as a likely single member with 99.5% probability.