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Paper: Sagittarius Dwarf Spheroidal and M54 in the 1612 MHz OH Line
Volume: 497, Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time
Page: 501
Authors: Sjouwerman, L. O.; Claussen, M. J.
Abstract: We have observed the M 54 region in the Sagittarius Dwarf Spheroidal galaxy with the VLA for 1612 MHz OH emission in an attempt to detect OH/IR stars outside the Galaxy and LMC. With an rms noise of ∼1 mJy/beam in a ∼1 km s-1 channel, we do not, however, detect any line sources.
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