<h1>Wannier, Peter G.</h1>
<h2>Combined from <a href="https://authors.library.caltech.edu">CaltechAUTHORS</a></h2>
<ul>
<li>Phillips, T. G. and Knapp, G. R., el al. (1981) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20170308-113011537">Temperatures of galactic molecular clouds showing CO self-absorption</a>; Astrophysical Journal; Vol. 245; 512-528; <a href="https://doi.org/10.1086/158826">10.1086/158826</a></li>
<li>Huggins, P. J. and Phillips, T. G., el al. (1979) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20170303-153447009">The detection of the J = 3-2 lines of HCN, HNC, and HCO^+ in the Orion molecular cloud</a>; Astrophysical Journal; Vol. 227; 441-445; <a href="https://doi.org/10.1086/156750">10.1086/156750</a></li>
<li>Scoville, N. Z. and Irvine, W. M., el al. (1977) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20190403-153007434">CO emission from supernova remnants</a>; Astrophysical Journal; Vol. 216; 320-328; <a href="https://doi.org/10.1086/155473">10.1086/155473</a></li>
</ul>