1. Galactic Interstellar Sulfur Isotopes: A Radial 32S/34S Gradient?
- Author
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Yu, H. Z., Zhang, J. S., Henkel, C., Yan, Y. T., Liu, W., Tang, X. D., Langer, N., Luan, T. C., Chen, J. L., Wang, Y. X., Deng, G. G., and Zou, Y. P.
- Subjects
SULFUR isotopes ,CARBON isotopes ,LEAD isotopes ,SOLAR system ,INTERSTELLAR medium ,GALACTIC center ,STANDARD deviations - Abstract
We present observations of
12 C32 S,12 C34 S,13 C32 S, and12 C33 S J = 2−1 lines toward a large sample of massive star-forming regions by using the Arizona Radio Observatory 12 m telescope and the IRAM 30 m. Taking new measurements of the carbon12 C/13 C ratio, the32 S/34 S isotope ratio was determined from the integrated13 C32 S/12 C34 S line intensity ratios for our sample. Our analysis shows a32 S/34 S gradient from the inner Galaxy out to a galactocentric distance of 12 kpc. An unweighted least-squares fit to our data yields32 S/34 S = (1.56 ± 0.17)DGC + (6.75 ± 1.22) with a correlation coefficient of 0.77. Errors represent 1σ standard deviations. Testing this result by (a) excluding the Galactic center region, (b) excluding all sources with C34 S opacities >0.25, (c) combining our data and old data from previous study, and (d) using different sets of carbon isotope ratios leads to the conclusion that the observed32 S/34 S gradient is not an artifact but persists irrespective of the choice of sample and carbon isotope data. A gradient with rising32 S/34 S values as a function of galactocentric radius implies that the solar system ratio should be larger than that of the local interstellar medium. With the new carbon isotope ratios, we indeed obtain a local32 S/34 S isotope ratio about 10% below the solar system one, as expected in the case of decreasing32 S/34 S ratios with time and increased amounts of stellar processing. However, taking older carbon isotope ratios based on a lesser amount of data, such a decrease is not seen. No systematic variation of34 S/33 S ratios along galactocentric distance was found. The average value is 5.9 ± 1.5, the error denoting the standard deviation of an individual measurement. [ABSTRACT FROM AUTHOR]- Published
- 2020
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