The origin of R CrA variability: A complex triple system hosting a disk
E. Sissa, R. Gratton, J.M. Alcala, S. Desidera, S. Messina, D. Mesa,, V. D'Orazi, E. Rigliaco

TL;DR
This study reveals that R CrA is a young, highly absorbed binary system with a circumbinary disk, and suggests its variability is due to disk precession and increasing absorption, indicating a complex triple-star system.
Contribution
It models the periodic variability of R CrA as caused by a binary with a circumbinary disk, providing new insights into its structure and evolution.
Findings
R CrA is a young (~1.5 Myr) binary with high absorption.
The variability is explained by partial attenuation from a circumbinary disk.
The system may be a triple with a precessing disk caused by a companion.
Abstract
R~CrA is the brightest member of the Coronet star forming region and it is the closest Herbig AeBe star with a spectrum dominated by emission lines. Its luminosity has been monitored since the end of the 19th century, but the origin of its variability, which shows a stable period of ~days, is still unknown. We studied photometric and spectroscopic data for this star to investigate the nature of the variability of R~CrA. We exploited the fact that near infrared luminosity of the Herbig AeBe stars is roughly proportional to the total luminosity of the stars to derive the absorption, and then mass and age of R~CrA. In addition, we model the periodic modulation of the light curve as due to partial attenuation of a central binary by a circumbinary disk. This model reproduces very well the observations. We found that the central object in R~CrA is a very young ($1.5\pm…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Astro and Planetary Science
