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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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