Implications of the ISO LWS Spectrum of the Prototypical Ultraluminous Galaxy ARP 220. Fischer, J., Satyapal, S., Melnick, G., Cox, P., Cernicharo, J., Luhman, M., Stacey, G., Smith, H., Lord, S., & Greenhouse, M. In American Astronomical Society Meeting Abstracts, volume 191, pages 89.03, December, 1997.
bibtex   
@INPROCEEDINGS{1997AAS...191.8903F,
       author = {{Fischer}, J. and {Satyapal}, S. and {Melnick}, G. and {Cox}, P. and {Cernicharo}, J. and {Luhman}, M.~L. and {Stacey}, G.~J. and {Smith}, H.~A. and {Lord}, S.~D. and {Greenhouse}, M.~A.},
        title = "{Implications of the ISO LWS Spectrum of the Prototypical Ultraluminous Galaxy ARP 220}",
    booktitle = {American Astronomical Society Meeting Abstracts},
         year = 1997,
       series = {American Astronomical Society Meeting Abstracts},
       volume = {191},
        month = dec,
          eid = {89.03},
        pages = {89.03},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1997AAS...191.8903F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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