Spectroscopic infrared extinction mapping as a probe of grain growth in IRDCs

Abstract

We present spectroscopic tests of MIR to FIR extinction laws in IRDC G028.36+00.07, a potential site of massive star and star cluster formation. Lim & Tan (2014) developed methods of FIR extinction mapping of this source using $Spitzer$-MIPS $24\mu \mathrm{m}$ and $Herschel$-PACS $70\mu \mathrm{m}$ images, and by comparing to MIR $Spitzer$-IRAC $3$--$8\mu \mathrm{m}$ extinction maps, found tentative evidence for grain growth in the highest mass surface density regions. Here we present results of spectroscopic infrared extinction (SIREX) mapping using $Spitzer$-IRS (14 to $38\mu \mathrm{m}$) data of the same IRDC. These methods allow us to first measure the SED of the diffuse Galactic ISM that is in the foreground of the IRDC. We then carry out our primary investigation of measuring the MIR to FIR opacity law and searching for potential variations as a function of mass surface density within the IRDC. We find relatively flat, featureless MIR-FIR opacity laws that lack the $\sim 12\mu \mathrm{m}$ and $\sim 35\mu \mathrm{m}$ features associated with the thick water ice mantle models of Ossenkopf & Henning (1994). Their thin ice mantle models and the coagulating aggregate dust models of Ormel et al. (2011) are a generally better match to the observed opacity laws. We also find evidence for generally flatter MIR to FIR extinction laws as mass surface density increases, strengthening the evidence for grain and ice mantle growth in higher density regions.

12 pages, 12 Figures, 1 Table, Accepted to be published to ApJ

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Cited by in corpus (3)

• Temperature structure and kinematics of the IRDC G035.39-00.33
• The Distribution of Mass Surface Densities in a High-Mass Protocluster
• Deuterium Chemodynamics of Massive Pre-Stellar Cores