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Acetylene bands observed in carbon stars: a laboratory study and an illustrative example of its application to IRC+10216

Journal Article · · Astrophys. J., Suppl. Ser.; (United States)
DOI:https://doi.org/10.1086/190808· OSTI ID:6052214
Acetylene (C/sub 2/H/sub 2/) has been identified as a constituent of the atmospheres of cool carbon stars based on Fourier transform stellar spectra in the near-infrared. To interpret these astrophysical data on a quantitative basis, a systematic laboratory study of the absorption spectrum of acetylene occurring in this spectral region has been made at a resolution of approx.0.03 cm/sup -1/, both at room temperature and at an elevated temperature of 160 /sup 0/C. Interpretation of the acetylene lines in the 3 ..mu..m region has led to the identification of 27 vibration-rotation bands which have been assigned to transitions between 41 different vibrational states of /sup 12/C/sub 2/H/sub 2/ and /sup 12/C/sup 13/CH/sub 2/, and absolute strengths were measured for 101 selected unblended spectral lines distributed among some of the stronger bands including the 0010/sup 0/0/sup 0/-0000/sup 0/0/sup 0/ band of /sup 12/C/sup 13/CH/sub 2/. In addition, the integrated strengths of the Q-branches of the 1000/sup 0/1/sup 1/-0000/sup 0/0/sup 0/ band at 4091 cm/sup -1/ and the 0100/sup 0/1/sup 1/-0000/sup 0/0/sup 0/ band at 2701 cm/sup -1/ of /sup 12/C/sub 2/H/sub 2/ were measured, and by comparing with the stellar data for IRC+10216, an estimate has been made for the acetylene column density in the circumstellar shell of this carbon star.
Research Organization:
Department of Physics, College of William and Mary
OSTI ID:
6052214
Journal Information:
Astrophys. J., Suppl. Ser.; (United States), Journal Name: Astrophys. J., Suppl. Ser.; (United States) Vol. 49:4; ISSN APJSA
Country of Publication:
United States
Language:
English