Fig. 1 from Effelsberg Observations of Excited‐State (6.0 GHz) OH in Supernova Remnants and W3(OH)

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Effelsberg Observations of Excited‐State (6.0 GHz) OH in Supernova Remnants and W3(OH)

Authors: Vincent L. Fish, Loránt O. Sjouwerman, and Ylva M. Pihlström

Fish, Sjouwerman, & Pihlström 2007 The Astrophysical Journal Letters 670 L117.

Provider: AAS Journals

Caption: Fig. 1.

Spectra of the 6016 and 6049 MHz transitions in W3(OH). Emission in the 6049 MHz transition is stronger than absorption in the 6016 MHz transition. A single‐Gaussian fit to the emission is narrower than a similar fit to the absorption.

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