{ "id": "1208.4097", "version": "v2", "published": "2012-08-20T20:00:00.000Z", "updated": "2012-08-22T18:36:37.000Z", "title": "There are no starless massive proto-clusters in the first quadrant of the Galaxy", "authors": [ "A. Ginsburg", "E. Bressert", "J. Bally", "C. Battersby" ], "comment": "Accepted to ApJL. See also Bressert et al 2012, http://arxiv.org/abs/1208.3472", "categories": [ "astro-ph.GA" ], "abstract": "We search the lambda = 1.1 mm Bolocam Galactic Plane Survey for clumps containing sufficient mass to form ~10^4 M\\odot star clusters. 18 candidate massive proto-clusters are identified in the first Galactic quadrant outside of the central kiloparsec. This sample is complete to clumps with mass M(clump) > 10^4 M_sun and radius r < 2.5 pc. The overall Galactic massive cluster formation rate is CFR(M_cluster > 10^4) ~ 5 Myr^-1, which is in agreement with the rates inferred from Galactic open clusters and M31 massive clusters. We find that all massive proto-clusters in the first quadrant are actively forming massive stars and place an upper limit of t_starless < 0.5 Myr on the lifetime of the starless phase of massive cluster formation. If massive clusters go through a starless phase with all of their mass in a single clump, the lifetime of this phase is very short.", "revisions": [ { "version": "v2", "updated": "2012-08-22T18:36:37.000Z" } ], "analyses": { "keywords": [ "first quadrant", "starless massive proto-clusters", "mm bolocam galactic plane survey", "massive cluster", "first galactic quadrant outside" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/758/2/L29", "journal": "The Astrophysical Journal", "year": 2012, "month": "Oct", "volume": 758, "number": 2 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2012ApJ...758L..29G", "inspire": 1128407 } } }