Do the W44 and W28 molecular clouds show evidence of a shock

• 1 January 1983
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 264, 141-151
• https://doi.org/10.1086/160582

Abstract

Keywords

• H LINES
• HYDROXYL EMISSION
• MOLECULAR CLOUDS
• SHOCK WAVES
• SUPERNOVA REMNANTS
• ABUNDANCE
• ASTRONOMICAL MAPS
• MOLECULAR EXCITATION
• MOLECULAR SPECTRA
• OPTICAL THICKNESS
• SPECTRAL LINE WIDTH