2001. The American Astronomical Society. All rights reserved. Printed in U.S.A. MILLIMETER-WAVE APERTURE SYNTHESIS IMAGING OF VEGA: EVIDENCE FOR A RING ARC AT 95 AU

We present the first millimeter-wave aperture synthesis map of dust around a main-sequence star. A 3 resolution image of 1.3 mm continuum emission from Vega reveals a clump of emission 12 from the star at a position angle (P.A.) of 45, consistent with the location of maximum 850 mm emission in a lower resolution James Clerk Maxwell Telescope/Submillimeter Common-User Bolometric Array (SCUBA) map. The flux density is 4.0 mJy. Adjacent 1.3 mm peaks with flux densities of and mJy are located 14 and 130.9 3.4 1.0 2.8 0.9 from the star at P.A.’s of 67 and 18, respectively. An arclike bridge connects the two strongest peaks. There is an additional mJy peak to the southwest, 11 from the star at, and a marginal detection,2.4 0.8 P.A.p 215 mJy, at the stellar position, consistent with photospheric emission. An extrapolation from the 850 mm1.4 0.5 flux, assuming, agrees well with the total detected flux for Vega at 1.3 mm and implies a dust2.8F ∝ l1.3–0.85 mm emissivity index b of 0.8 We conclude that we have detected all but a very small fraction of the dust imaged by SCUBA in our aperture synthesis map and that these grains are largely confined to segments of a ring of radius 95 AU. Subject headings: circumstellar matter — planetary systems: formation — planetary systems: protoplanetary disks — stars: individual (a Lyrae) 1