First Interstellar HCO${}^{+}$ Maser

Abstract

A previously unseen maser in the J = 1 - 0 transition of HCO${}^{+}$ has been detected by the Combined Array for Millimeter-wave Astronomy (CARMA). A sub-arcsecond map was produced of the 2 arcmin${}^2$ region around DR21(OH), which has had previous detections of OH and methanol masers. This new object has remained undetected until now due to its extremely compact size. The object has a brightness temperature of $>$ 2500 K and a FWHM linewidth of 0.497 km s${}^{-1}$, both of which suggest non-thermal line emission consistent with an unsaturated maser. This object coincides in position and velocity with the methanol maser named DR21(OH)-1 by \citet{plambeck90}. No compact HCO${}^{+}$ emission was present in the CARMA data towards the other methanol masers described in that paper. These new results support the theory introduced in \citet{plambeck90} that these masers likely arise from strong outflows interacting with low mass, high density pockets of molecular gas. This is further supported by recent observations of a CO outflow by \citet{zapata12} that traces the outflow edges and confirms that the maser position lies along the edge of the outflow where interaction with molecular tracers can occur.

4 pages, 3 figures, accepted by ApJL on September 10, 2012

References in corpus (6)

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Cited by in corpus (1)

• DR 21(OH): a highly fragmented, magnetized, turbulent dense core