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Identification of Main-Sequence Stars with Mid-Infrared Excesses Using GLIMPSE: β Pictoris Analogs?

journal contribution
posted on 2023-05-16, 17:45 authored by Uzpen, B, Kobulnicky, HA, Olsen, KAG, Clemens, DP, Laurance, TL, Meade, MR, Babler, BL, Indebetouw, R, Whitney, BA, Watson, C, Wolfire, MG, Wolff, MJ, Benjamin, RA, Bania, TM, Cohen, M, Devine, KE, John DickeyJohn Dickey, Heitsch, F, Jackson, JM, Marston, AP, Mathis, JS, Mercer, EP, Stauffer, JR, Stolovy, SR, Backman, DE, Churchwell, E
Spitzer IRAC 3.6-8 μm photometry obtained as part of the GLIMPSE survey has revealed mid-infrared excesses for 33 field stars with known spectral types in a 1.2 deg2 field centered on the southern Galactic H II region RCW 49. These stars comprise a subset of 184 stars with known spectral classification, most of which were preselected to have unusually red IR colors. We propose that the mid-IR excesses are caused by circumstellar dust disks that are either very late remnants of stellar formation or debris disks generated by planet formation. Of these 33 stars, 29 appear to be main-sequence stars on the basis of optical spectral classifications. Five of the 29 main-sequence stars are O or B stars with excesses that can be plausibly explained by thermal bremsstrahlung emission, and four are post-main-sequence stars. The lone O star is an O4 V((f)) at a spectrophotometric distance of 3233-535 +540 pc and may be the earliest member of the Westerlund 2 cluster. Of the remaining 24 main-sequence stars, 18 have spectral energy distributions that are consistent with hot dusty debris disks, a possible signature of planet formation. Modeling the excesses as blackbodies demonstrates that the blackbody components have fractional bolometric disk-to-star luminosity ratios, L IR/L*, ranging from 10-3 to 10-2 with temperatures ranging from 220 to 820 K. The inferred temperatures are more consistent with asteroid belts than with the cooler temperatures expected for Kuiper belts. Mid-IR excesses are found in all spectral types from late B to early K. © 2005. The American Astronomical Society. All rights reserved.

History

Publication title

The Astrophysical Journal

Volume

629

Pagination

512-525

ISSN

0004-637X

Department/School

School of Natural Sciences

Publisher

The University of Chicago Press

Place of publication

Chicago, USA

Repository Status

  • Restricted

Socio-economic Objectives

Expanding knowledge in the physical sciences

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