Complex Organic Molecules in Diffuse Clouds Along the Line of Sight to Sgr B2

By Keith Cowing
Press Release
August 24, 2017
Filed under
Complex Organic Molecules in Diffuse Clouds Along the Line of Sight to Sgr B2
Sgr B2

Up to now, mostly relatively simple molecules have been detected in interstellar diffuse molecular clouds in our galaxy, but more complex species have been reported in the diffuse/translucent medium of a z = 0.89 spiral galaxy.

We aim at searching for complex organic molecules (COMs) in diffuse molecular clouds along the line of sight to Sgr B2(N), taking advantage of the high sensitivity and angular resolution of the Atacama Large Millimeter/submillimeter Array (ALMA). We use data acquired as part of the EMoCA survey performed with ALMA.

To analyse the absorption features of the molecules detected towards the ultracompact HII region K4 in Sgr B2(N), we calculate synthetic spectra for these molecules and fit their column densities, line widths, centroid velocities, and excitation temperatures. We report the detection of CH3OH, CH3CN, CH3CHO, HC3N, and NH2CHO in Galactic center (GC) diffuse clouds and CH3OH and CH3CN in a diffuse cloud in the Scutum arm. The chemical composition of one of the diffuse GC clouds is found to be similar to the one of the diffuse/translucent medium of the z=0.89 spiral galaxy.

The chemical processes leading to chemical complexity in the diffuse molecular ISM appear to have remained similar since z=0.89. As proposed in previous studies, the presence of COMs in diffuse molecular clouds may result from a cyclical interstellar process of cloud contraction and expansion between diffuse and dense states.

V. Thiel, A. Belloche, K. M. Menten, R. T. Garrod, H. S. P. Müller
(Submitted on 24 Aug 2017)

Comments: Accepted for publication as a letter in A&A, 5 pages, 3 figures
Subjects: Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:1708.07292 [astro-ph.GA] (or arXiv:1708.07292v1 [astro-ph.GA] for this version)
Submission history
From: Vivien Thiel
[v1] Thu, 24 Aug 2017 06:58:04 GMT (168kb,D)

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