Abstract
Abundance relationships between the interstellar NH molecule and other diatomic species are presented based on 10 currently available sightlines (two of them taken from the literature). Spacial correlations between column densities of diatomic molecules suggest that the NH molecule is more closely related to neutral species than it is to CH+. © 2009 RAS.
Author supplied keywords
Cite
CITATION STYLE
APA
Weselak, T., Galazutdinov, G. A., Beletsky, Y., & Krełowski, J. (2009). Interstellar NH molecule in translucent sightlines. Monthly Notices of the Royal Astronomical Society, 400(1), 392–397. https://doi.org/10.1111/j.1365-2966.2009.15466.x
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free