Differences

This shows you the differences between two versions of the page.

--- molecules:ism:me [2025/11/12 15:02] – mueller
+++ molecules:ism:me [2025/11/12 15:03] (current) – mueller
@@ Line 12: / Line 12: @@
 **[[https://doi.org/10.3847/2041-8213/ae0e6b|A Quest for Sulfur-bearing Refractory Species: Identification of CaS in the Interstellar Medium]]**\\
 //Astrophys. J. Lett.// **993**, Art. No. L42 (2025).\\
-Four transitions with //J// = 19 − 18 or 18 − 17 and //v// = 0 or 1 were observed with ALMA toward the G351.77-mm1 protostellar disk. Three lines are blended, but the one with //J// = 19 − 18 and //v// = 0 at 200.714 GHz is partially clear and the //J// = 18 − 17 and //v// = 1 at 189.261 GHz apparently helps to constrain //T//<sub>rot</sub> and the column density. //J// = 22 − 21, //v// = 0, at 232.372 GHz was covered by archival ALMA data, and the high-resolution recording suggests this line dominates at least part of the emission feature. The same extent as NaCl and the value of //T//<sub>rot</sub> can be viewed in support of the assignment. Slight caution may be advised nevertheless until further lines will have been detected.
+Four transitions with //J// = 19 − 18 or 18 − 17 and //v// = 0 or 1 were observed with ALMA toward the G351.77-mm1 protostellar disk. Three lines are blended, but the one with //J// = 19 − 18 and //v// = 0 at 200.714 GHz is partially clear and the //J// = 18 − 17 and //v// = 1 at 189.261 GHz apparently helps to constrain //T//<sub>rot</sub> and the column density. //J// = 22 − 21, //v// = 0, at 232.372 GHz was covered by archival ALMA data, and the high-resolution recording suggests this line dominates at least part of the emission feature. The same extent as NaCl and the value of //T//<sub>rot</sub> can be viewed in support of the assignment to CaS. Slight caution may be advised nevertheless until further lines will have been detected.
 \\