Huang and Thaddeus 1985
Huang, Y.-L., and P. Thaddeus, 1985: The Σ-D relation for shell-like supernova remnants. Astrophys. J., 295, L13-L16, doi:10.1086/184528.
A large fraction of Galactic supernova remnants, including a dozen shell-like remnants, can be associated with large molecular clouds or cloud complexes with well-determined distances. The Sigma-D relation for these shell-like remnants, derived using distances to the associated molecular clouds, shows substantially smaller scatter than previous relations and establishes a good distance scale for shell-like remnants from Type II events.
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Huang, Y.-L., and Thaddeus, P.: The Σ-D relation for shell-like supernova remnants, Astrophys. J., 295, L13-L16, doi:10.1086/184528, 1985.
Huang, Y.-L., and P. Thaddeus (1985), The Σ-D relation for shell-like supernova remnants, Astrophys. J., 295, L13-L16, doi:10.1086/184528.
Huang, Y.-L., and P. Thaddeus, 1985: The Σ-D relation for shell-like supernova remnants. Astrophys. J., 295, L13-L16, doi:10.1086/184528.
Huang, Y.-L., & Thaddeus, P. 1985, Astrophys. J., 295, L13, doi:10.1086/184528.
Huang Y-L, Thaddeus P. The Σ-D relation for shell-like supernova remnants, Astrophys J 1985;295:L13-L16. doi:10.1086/184528.
Y.-L. Huang, P. Thaddeus, Astrophys. J. 295, L13-L16, doi:10.1086/184528 (1985).
