{"paper":{"title":"The maser emitting structure and time variability of the SiS lines J=14-13 and 15-14 in IRC+10216","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Castro-Carrizo, C. S\\'anchez Contreras, G. Quintana-Lacaci, J. Cernicharo, J. P. Fonfr\\'ia, J. R. Pardo, L. Velilla Prieto, M. Ag\\'undez, M. Fern\\'andez-L\\'opez, M. Santander-Garc\\'ia, S. Curiel","submitted_at":"2018-05-14T15:11:48Z","abstract_excerpt":"We present new high angular resolution interferometer observations of the v=0 J=14-13 and 15-14 SiS lines towards IRC+10216, carried out with CARMA and ALMA. The maps, with angular resolutions of ~0.25\"and 0.55\", reveal (1) an extended, roughly uniform, and weak emission with a size of ~0.5\", (2) a component elongated approximately along the East-West direction peaking at ~0.13\" and 0.17\" at both sides of the central star, and (3) two blue- and red-shifted compact components peaking around 0.07\" to the NW of the star. We have modeled the emission with a 3D radiation transfer code finding that "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.05218","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":""},"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"}