Survey of Molecular Emission Lines in the WB 673 Interstellar Filament View Full Text


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Article Info

DATE

2020-05

AUTHORS

O. L. Ryabukhina, M. S. Kirsanova

ABSTRACT

—We report observations of molecular line emission toward dense clumps of the WB 673 interstellar filament: WB 668, WB 673, S233–IR, and G173.57+2.43. The observations were done with the 20-m telescope at the Onsala Space Observatory (Sweden). Maps of emission, column densities, and relative abundances of CO, N2H\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{ + }$$\end{document}, CS, HCN, and HNC molecules are presented. It was found that the molecular abundances decrease toward the peaks of molecular hydrogen column densities in the clumps. More... »

PAGES

394-405

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1134/s1063772920050030

DOI

http://dx.doi.org/10.1134/s1063772920050030

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1128247033


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