paper

The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE Data

arXiv:astro-ph/0406403 · doi:10.1086/426679

Abstract

We determine and tabulate A(lambda)/A(K), the wavelength dependence of interstellar extinction, in the Galactic plane for 1.25um<lambda<8.0um along two lines of sight: l~42 and l~284. The first is a relatively quiescent and unremarkable region; the second contains the giant HII region RCW 49 as well as a ``field'' region unrelated to the cluster and nebulosity. Areas near these Galactic longitudes were imaged at J, H, and K bands by 2MASS and at 3--8um by Spitzer for the GLIMPSE Legacy program. We measure the mean values of the color excess ratios (A(lambda)-A(K))/(A(J)-A(K)) directly from the color distributions of observed stars. The extinction ratio between two of the filters, e.g. A(J)/A(K), is required to calculate A(lambda)/A(K) from those measured ratios. We use the apparent JHK magnitudes of giant stars along our two sightlines, and fit the reddening as a function of magnitude (distance) to determine A(J)/kpc, A(K)/kpc, and A(J)/A(K). Our values of A(lambda)/A(K) show a flattening across the 3--8um wavelength range, roughly consistent with the Lutz 1996 extinction measurements derived for the sightline toward the Galactic center.

20pp, 6fig, accepted version: description of the method has been revised, results are unchanged, discussion of implications slightly expanded

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