{ "id": "1502.03109", "version": "v1", "published": "2015-02-10T21:00:27.000Z", "updated": "2015-02-10T21:00:27.000Z", "title": "Radio Continuum Observations of the Galactic Center: Photoevaporative Proplyd-like Objects near Sgr A*", "authors": [ "F. Yusef-Zadeh", "D. A. Roberts", "M. Wardle", "W. Cotton", "R. Schödel", "M. J. Royster" ], "comment": "13 pages, 4 figures, ApJL (in press)", "categories": [ "astro-ph.GA" ], "abstract": "We present radio images within 30$''$ of Sgr A* based on recent VLA observations at 34 GHz with 7.8 microJy sensitivity and resolution $\\sim88\\times46$ milliarcseconds (mas). We report 44 partially resolved compact sources clustered in two regions in the E arm of ionized gas that orbits Sgr A*. These sources have size scales ranging between ~50 and 200 mas (400 to 1600 AUs), and a bow-shock appearance facing the direction of Sgr A*. Unlike the bow-shock sources previously identified in the near-IR but associated with massive stars, these 34 GHz sources do not appear to have near-IR counterparts at 3.8 $\\mu$m. We interpret these sources as a candidate population of photoevaporative protoplanetary disks (proplyds) that are associated with newly formed low mass stars with mass loss rates ~10^{-7} - 10^{-6} solar mass per year and are located at the edge of a molecular cloud outlined by ionized gas. The disks are externally illuminated by strong Lyman continuum radiation from the ~100 OB and WR massive stars distributed within 10'' of Sgr A*. The presence of proplyds implies current in-situ star formation activity near Sgr A* and opens a window for the first time to study low mass star, planetary and brown dwarf formations near a supermassive black hole.", "revisions": [ { "version": "v1", "updated": "2015-02-10T21:00:27.000Z" } ], "analyses": { "keywords": [ "radio continuum observations", "photoevaporative proplyd-like objects", "in-situ star formation activity", "implies current in-situ star", "galactic center" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }