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To quantitatively understand the non-thermal emission process, accurate knowledge of the physical and orbital properties of the object is crucial. Here, we aim to investigate the orbital properties of the wide system and to constrain the inclinations of the inner and outer binaries, and with these the absolute masses of the system components."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1304.3457","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-04-11T20:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"31ecfe14cc503bfb7b62a463207225f45cbfc9c41abba910cd3b489020afc90c","abstract_canon_sha256":"3af64c590da6d45adec684a0a28ad36bb665fc38bf61646e11e1de77de7112c7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:33.691391Z","signature_b64":"+9uoJRy9B5ctCfeN51L3x48brgOBGmM/1MX+f7LomC4f6OrmbfpWZq433vQJCGUv3/exitGDjxc/Dj4PrkGwAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b1117e744298e58f505105b693af01eb7179a237e01aa53acb4b413838593b4","last_reissued_at":"2026-05-18T01:50:33.690682Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:33.690682Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Three-dimensional orbits of the triple-O stellar system HD 150136","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"E. Gosset, H. Sana, J.-B. Le Bouquin, L. Mahy, M. De Becker, O. Absil","submitted_at":"2013-04-11T20:00:01Z","abstract_excerpt":"Context. HD 150136 is a triple hierarchical system and a non-thermal radio emitter. It is formed by an O3-3.5 V + O5.5-6 V close binary and a more distant O6.5-7 V tertiary. So far, only the inner orbital properties have been reliably constrained.\n  Aims. To quantitatively understand the non-thermal emission process, accurate knowledge of the physical and orbital properties of the object is crucial. 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