Cummins et al. 1980

Cummins, S.E., M. Morris, and P. Thaddeus, 1980: On C₄H versus vibrationally excited CO in IRC+10216. Astrophys. J., 235, 886-888, doi:10.1086/157690.

The N = 12→11 doublet of ₄H in IRC+10216 is observed to be nearly symmetric; there is no evidence of a blend with vibrationally excited CO.

• Download PDF (Document is 305 kB; scanned, no OCR)
• PDF documents require a special viewer such as the free Adobe Reader.

Citation Styles

Show: ACP, AGU, AMS, ApJ, JQSRT, Science style

Cummins, S.E., Morris, M., and Thaddeus, P.: On C₄H versus vibrationally excited CO in IRC+10216, Astrophys. J., 235, 886-888, doi:10.1086/157690, 1980.

Cummins, S.E., M. Morris, and P. Thaddeus (1980), On C₄H versus vibrationally excited CO in IRC+10216, Astrophys. J., 235, 886-888, doi:10.1086/157690.

Cummins, S.E., M. Morris, and P. Thaddeus, 1980: On C₄H versus vibrationally excited CO in IRC+10216. Astrophys. J., 235, 886-888, doi:10.1086/157690.

Cummins, S.E., Morris, M., & Thaddeus, P. 1980, Astrophys. J., 235, 886, doi:10.1086/157690.

Cummins SE, Morris M, Thaddeus P. On C₄H versus vibrationally excited CO in IRC+10216, Astrophys J 1980;235:886-888. doi:10.1086/157690.

S.E. Cummins, M. Morris, P. Thaddeus, Astrophys. J. 235, 886-888, doi:10.1086/157690 (1980).