Hostname: page-component-8448b6f56d-jr42d Total loading time: 0 Render date: 2024-04-24T18:49:20.740Z Has data issue: false hasContentIssue false

Formation, Evolution and Destruction of Possible DIB Carriers: Dirty Molecular Hydrogen Ice Clusters

Published online by Cambridge University Press:  21 February 2014

D. K. Lynch
Affiliation:
Thule Scientific, P.O. Box 953, Topanga CA 90290, USA email: dave@thulescientific.com
L. S. Bernstein
Affiliation:
Spectral Sciences Inc., 4 Fourth Avenue, Burlington, MA 01803, USA email: larry@spectral.com
F. O. Clark
Affiliation:
Spectral Sciences Inc., 4 Fourth Avenue, Burlington, MA 01803, USA email: larry@spectral.com
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We suggest that the diffuse interstellar bands (DIBs) are absorption lines arising from electronic transitions in molecular clusters primarily composed of a single molecule, atom, or ion (“seed”), embedded in a single-layer shell of H2 molecules (Bernstein et al. 2013). We refer to these clusters as CHCs (Contaminated H2 Clusters). CHCs arise from cm-sized, dirty H2 ice balls, called CHIMPs (Contaminated H2 Ice Macro-Particles), formed in cold, dense, Giant Molecular Clouds (GMCs), and later released into the interstellar medium (ISM) upon GMC disruption. Absorption by the CHIMP of a UV photon releases CHCs. CHCs produce DIBs when they absorb optical photons. When this occurs, the absorbed photon energy disrupts the CHC.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Bernstein, L. S, Clark, F. O., & Lynch, D. K. 2013, ApJ, 768, 84CrossRefGoogle Scholar
Draine, B. T. 1978, ApJS, 36, 595CrossRefGoogle Scholar
Jura, M. 1974, ApJ, 191, 375CrossRefGoogle Scholar
Murray, N., Quataert, E. & Thompson, T. A. 2010, ApJ, 709, 191Google Scholar
Oort, J. H. 1954, BAN, 12, 177Google Scholar