{"paper":{"title":"The GRAVITY young stellar object survey XIV : Investigating the magnetospheric accretion-ejection processes in S CrA N","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. Caratti o Garatti, A. Drescher, A. Eckart, A. Soulain, C. Dougados, C. Straubmeier, D. Lutz, D. Ribeiro, E. Alecian, E. Gendron, E. Sturm, E. van Dishoeck, F. Eisenhauer, F. Mang, F. Vincent, F. Widmann, G. Bourdarot, G. Perrin, GRAVITY Collaboration: H. Nowacki, H. Feuchtgruber, J. A. Wojtczak, J.-B. Le Bouquin, J. Bouvier, J.-P. Berger, J. S\\'anchez-Berm\\'udez, J. Shangguan, K. Perraut, L. Jocou, L. Labadie, L. Tacconi, M. Benisty, M. Fabricius, M. Sadun Bordoni, N. Kurtovic, N. M. F\\\"orster-Schreiber, P. Caselli, P. Garcia, P. Kervella, R. Davies, R. Garcia Lopez, R. Genzel, S. Gillessen, S. Grant, S. Lacour, S. Rabien, S. Scheithauer, S. Spezzano, T. Henning, T. Ott, T. Paumard, T. Shimizu, V. Ganci, V. Lapeyr\\`ere, W. Brandner, Y. Cl\\'enet","submitted_at":"2024-08-05T10:57:00Z","abstract_excerpt":"The dust- and gas-rich protoplanetary disks around young stellar systems play a key role in star and planet formation. While considerable progress has recently been made in probing these disks on large scales of a few tens of astronomical units (au), the central au needs to be more investigated. We aim at unveiling the physical processes at play in the innermost regions of the strongly accreting T Tauri Star S CrA N by means of near-infrared interferometric observations. The K-band continuum emission is well reproduced with an azimuthally-modulated dusty ring. As the star alone cannot explain "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.02374","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2408.02374/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}