{ "id": "2310.15491", "version": "v1", "published": "2023-10-24T03:39:02.000Z", "updated": "2023-10-24T03:39:02.000Z", "title": "Early Planet Formation in Embedded Disks (eDisk) X: Compact Disks, Extended Infall, and a Fossil Outburst in the Class I Oph IRS43 Binary", "authors": [ "Suchitra Narayanan", "Jonathan P. Williams", "John J. Tobin", "Jes K. Jorgensen", "Nagayoshi Ohashi", "Zhe-Yu Daniel Lin", "Merel L. R. van't Hoff", "Zhi-Yun Li", "Adele L. Plunkett", "Leslie W. Looney", "Shigehisa Takakuwa", "Hsi-Wei Yen", "Yusuke Aso", "Christian Flores", "Jeong-Eun Lee", "Shih-Ping Lai", "Woojin Kwon", "Itziar de Gregorio-Monsalvo", "Rajeeb Sharma", "Chang Won Lee" ], "comment": "Paper 10 of the ALMA eDisk Large Program. Accepted for publication in ApJ", "categories": [ "astro-ph.SR", "astro-ph.EP" ], "abstract": "We present the first results from the Early Planet Formation in Embedded Disks (eDisk) ALMA Large Program toward Oph IRS43, a binary system of solar mass protostars. The 1.3 mm dust continuum observations resolve a compact disk, ~6au radius, around the northern component and show that the disk around the southern component is even smaller, <~3 au. CO, 13CO, and C18O maps reveal a large cavity in a low mass envelope that shows kinematic signatures of rotation and infall extending out to ~ 2000au. An expanding CO bubble centered on the extrapolated location of the source ~130 years ago suggests a recent outburst. Despite the small size of the disks, the overall picture is of a remarkably large and dynamically active region.", "revisions": [ { "version": "v1", "updated": "2023-10-24T03:39:02.000Z" } ], "analyses": { "keywords": [ "early planet formation", "oph irs43 binary", "compact disk", "embedded disks", "fossil outburst" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }