NaCl lines in the spectral windows covered by the ALMA observations.
|[GHz]||[cm-1]||s-1||[mJy beam-1 km s-1]||[“×”, PA]|
|v = 1 J = 24−23||309.787||480.09||0.017||19||0.232 × 0.131, 28.27°||unblended|
|v = 0 J = 24−23||312.110||119.83||0.013||30||0.239 × 0.134, 29.48°||unblended|
|v = 1 J = 25−24||322.650||490.42||0.019||27||0.222 × 0.126, 27.55°||red wing slightly blended by TiO2 line|
|v = 0 J = 25−24||325.069||130.24||0.015||195||0.217 × 0.119, 29.27°||blue wing blended by H2O maser|
|+ blend with SiS v = 1J = 18−17|
Notes. Listed are the transition, rest frequency, lower state energy, Einstein A-values from CDMS, the rms noise, the synthesized beam, and comments concerning line blending.
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