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[en] Sgr B2 is a well-known star-forming molecular cloud complex in the Galactic center region showing evidence of high energy activity as traced by the Kα neutral Fe i line at 6.4 keV, as well as GeV and TeV γ-ray emission. Here, we present Very Large Array and GMRT observations with respective resolutions of ≈ 3.''5 x 1.''2 and 25'' x 25'' and report the detection of an OH(1720 MHz) maser, with no accompanying OH 1665, 1667, and 1612 MHz maser emission.
Journal
Astrophysical Journal Letters; ISSN 2041-8205; 
; v. 819(2); [6 p.]
; v. 819(2); [6 p.]