Far-infrared excess emission as a tracer of disk-halo interaction

Abstract

Given the current and past star-formation in the Milky Way in combination with the limited gas supply, the re-fuelling of the reservoir of cool gas is an important aspect of Galactic astrophysics. The infall of \ion{H}{i} halo clouds can, among other mechanisms, contribute to solving this problem. We study the intermediate-velocity cloud IVC135+54 and its spatially associated high-velocity counterpart to look for signs of a past or ongoing interaction. Using the Effelsberg-Bonn \ion{H}{i} Survey data, we investigated the interplay of gas at different velocities. In combination with far-infrared Planck and IRIS data, we extended this study to interstellar dust and used the correlation of the data sets to infer information on the dark gas. The velocity structure indicates a strong compression and deceleration of the infalling high-velocity cloud (HVC), associated with far-infrared excess emission in the intermediate-velocity cloud. This excess emission traces molecular hydrogen, confirming that IVC135+54 is one of the very few molecular halo clouds. The high dust emissivity of IVC135+54 with respect to the local gas implies that it consists of disk material and does not, unlike the HVC, have an extragalactic origin. Based on the velocity structure of the HVC and the dust content of the IVC, a physical connection between them appears to be the logical conclusion. Since this is not compatible with the distance difference between the two objects, we conclude that this particular HVC might be much closer to us than complex C. Alternatively, the indicators for an interaction are misleading and have another origin.

11 pages, 10 figures, accepted for publication in A&A

References in corpus (8)

• Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample
• Cold gas accretion in galaxies
• Accretion of gas onto nearby spiral galaxies
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Cited by in corpus (5)

• HI4PI: A full-sky HI survey based on EBHIS and GASS
• Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds
• All-sky census of Galactic high-latitude molecular intermediate-velocity clouds
• Maps of the number of HI clouds along the line of sight at high galactic latitude
• High-resolution HI and CO observations of high-latitude intermediate-velocity clouds