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The MGRO J2019+37 region is one of the brightest sources in the sky at TeVenergies. It was detected in the 2 year HAWC catalog as 2HWC J2019+367 and herewe present a detailed study of this region using data from HAWC. This analysisresolves the region into two sources: HAWC J2019+368 and HAWC J2016+371. Weassociate HAWC J2016+371 with the evolved supernova remnant CTB 87, althoughits low significance in this analysis prevents a detailed study at this time.An investigation of the morphology (including possible energy dependentmorphology) and spectrum for HAWC J2019+368 is the focus of this work. Weassociate HAWC J2019+368 with PSR J2021+3651 and its X-ray pulsar wind nebula,the Dragonfly nebula. Modeling the spectrum measured by HAWC and Suzaku revealsa $\sim$7 kyr pulsar and nebula system producing the observed emission at X-rayand ${\gamma}$-ray energies.

Spectrum and Morphology of the Very-High-Energy Source HAWC J2019+368