RX Gru is a pre-main-sequence eclipsing binary with twin components of mass ~1 solar mass each, age ~28 Myr, and a circumbinary companion of minimum mass 89 Mjup in a 23.8-year orbit.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
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astro-ph.SR 2years
2025 2verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
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RX Gru: a short-period pre-main-sequence eclipsing binary with a distant circumbinary companion
RX Gru is a pre-main-sequence eclipsing binary with twin components of mass ~1 solar mass each, age ~28 Myr, and a circumbinary companion of minimum mass 89 Mjup in a 23.8-year orbit.
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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.