Wilson et al. 1971
Wilson, R.W., A.A. Penzias, K.B. Jefferts, M. Kutner, and P. Thaddeus, 1971: Discovery of interstellar silicon monoxide. Astrohys. J., 167, L97-L100, doi:10.1086/180769.
Line emission attributed to the J=3→2 rotational transition of SiO has been detected in Sgr B2, at a radial velocity comparable to that of other molecules; the estimated column number density of SiO is 4×1013 /cm2. The line has not been found in Ori A, IRC+10216, Sgr A, W51, DR21, or NML Cyg.
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Wilson, R.W., Penzias, A.A., Jefferts, K.B., Kutner, M., and Thaddeus, P.: Discovery of interstellar silicon monoxide, Astrohys. J., 167, L97-L100, doi:10.1086/180769, 1971.
Wilson, R.W., A.A. Penzias, K.B. Jefferts, M. Kutner, and P. Thaddeus (1971), Discovery of interstellar silicon monoxide, Astrohys. J., 167, L97-L100, doi:10.1086/180769.
Wilson, R.W., A.A. Penzias, K.B. Jefferts, M. Kutner, and P. Thaddeus, 1971: Discovery of interstellar silicon monoxide. Astrohys. J., 167, L97-L100, doi:10.1086/180769.
Wilson, R.W., Penzias, A.A., Jefferts, K.B., Kutner, M., & Thaddeus, P. 1971, Astrohys. J., 167, L97, doi:10.1086/180769.
Wilson RW, Penzias AA, Jefferts KB, Kutner M, Thaddeus P. Discovery of interstellar silicon monoxide, Astrohys J 1971;167:L97-L100. doi:10.1086/180769.
R.W. Wilson, A.A. Penzias, K.B. Jefferts, M. Kutner, P. Thaddeus, Astrohys. J. 167, L97-L100, doi:10.1086/180769 (1971).
