ALMA spectral line and imaging survey of a low and a high mass-loss rate AGB star between 335 and 362 GHz

Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/201732216e]

Table 5

Frequencies (in GHz) of the unidentified lines.

335.993	336.307	336.471	336.815	336.973
337.421	338.170	338.447	338.520	338.677
338.814	339.103	339.398	339.417	340.787
341.141	341.233	344.223	344.719	345.020
345.086	345.420	346.120	346.196	346.954
347.221	347.956	348.117	348.256	348.497
348.525	348.634	348.878	348.998	349.530
349.890	349.970	350.145	350.475	350.356
350.559	350.810	351.049	351.512	351.581
351.790	351.920	352.034	352.074	352.502
353.570	353.796	355.284	355.875	355.967
356.461	356.462	356.933	356.974	357.767
358.468	358.680	359.660	361.596	361.734
361.896

Notes. Frequencies written in boldface refer to lines detected in both IK Tau and R Dor, in italics to spectral lines only detected in IK Tau, and in normal font only detected in R Dor.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.