Year: 2025
Type: preprint
Abstract: T CrA is a Herbig Ae-type young star in a complex circumstellar environment; it includes a circumstellar disk, accretion streamers, jets, and outflows. It has long been suspected to be a binary. However, until now, there has been no direct detection of a companion. Here we present new VLTI/MATISSE L- and N-band observations of T CrA taken between 2023 May and 2024 August with the aim of testing the binary nature of the system. We modeled the data with a geometric model using the Python tool oimodeler. We detected a companion (T CrA B) with a projected separation of $\Delta r = 153.2 \pm 1.2$ mas ($\approx 23$ au) toward the west direction at a position angle of $275.4 \pm 0.1^\circ$, in 2024 May-August. Our results support that the companion has a nearly edge-on orbit that is highly misaligned with respect to the circumprimary disk. Such a configuration could cause warping and tearing of the disk around the primary, which has been proposed by recent studies. In the L band the companion is extended, with a full width at half maximum (FWHM) size of $\sim 1$ au, suggesting that the emission comes from a disk around the secondary star. The companion flux is 0.2-0.3 Jy in the L band, and 0.2-0.7 Jy in the N band, accounting for 4-20% of the total emission at those wavelengths. The SED of the companion is compatible with thermal radiation of warm dust (600-800 K).
Source: arXiv (Cornell University)
Authors: Varga, J., Matter, A., Millour, F., Weigelt, G., van Boekel, R., Lopez, B., Lykou, F., K\'osp\'al, \'A, Chen, L., Boley, P. A., Wolf, S., Hogerheijde, M., Mo\'or, A., \'Abrah\'am, P., Augereau, J. -C., de Miera, F. Cruz-Saenz, Danchi, W. -C., Henning, Th., Juh\'asz, T., Priolet, P., Scheuck, M., Scigliuto, J., van Haastere, L., Zwicky, L.
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W6979340950
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