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Millimeter-Wave Aperture Synthesis Imaging of Vega: Evidence for a Ring Arc at 95 AU

Koerner, D. W. and Sargent, A. I. and Ostroff, N. A. (2001) Millimeter-Wave Aperture Synthesis Imaging of Vega: Evidence for a Ring Arc at 95 AU. Astrophysical Journal, 560 (2). L181-L184. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20190507-134433707

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Abstract

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 μm emission in a lower resolution James Clerk Maxwell Telescope/Submillimeter Common-User Bolometric Array (SCUBA) map. The flux density is 4.0 ± 0.9 mJy. Adjacent 1.3 mm peaks with flux densities of 3.4 ± 1.0 and 2.8 ± 0.9 mJy are located 14'' and 13'' from the star at P.A.'s of 67° and 18°, respectively. An arclike bridge connects the two strongest peaks. There is an additional 2.4 ± 0.8 mJy peak to the southwest, 11'' from the star at P.A. = 215°, and a marginal detection, 1.4 ± 0.5 mJy, at the stellar position, consistent with photospheric emission. An extrapolation from the 850 μm flux, assuming F_(1.3-0.85 mm) ∝ λ^(-2.8), agrees well with the total detected flux for Vega at 1.3 mm and implies a dust emissivity index β 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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/324226DOIArticle
https://arxiv.org/abs/astro-ph/0109424arXivDiscussion Paper
ORCID:
AuthorORCID
Sargent, A. I.0000-0002-4633-5098
Additional Information:© 2001 The American Astronomical Society. Received 2001 August 14; accepted 2001 September 6; published 2001 September 25. We are grateful to all OVRO postdoctoral scholars and visiting astronomers who helped in acquiring the data, but especially to Kartik Sheth. The OVRO millimeter array is supported by the NSF through grant AST 99-8154. OVRO research on other solar systems is also supported by the Norris Planetary Origins Project and NASA Origins grant NAG5-9530.
Funders:
Funding AgencyGrant Number
NSFAST 99-81546
Norris Planetary Origins ProjectUNSPECIFIED
NASANAG5-9530
Subject Keywords:circumstellar matter—planetary systems: formation— planetary systems: protoplanetary disks—stars: individual (α Lyrae)
Issue or Number:2
Record Number:CaltechAUTHORS:20190507-134433707
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190507-134433707
Official Citation:D. W. Koerner et al 2001 ApJ 560 L181
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95309
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:07 May 2019 20:55
Last Modified:03 Oct 2019 21:12

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