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We present a study of the star 2MASS J22472238+5801214 with the aim ofidentifying its true nature which has hitherto been uncertain. This object,which is a member of the young cluster NGC 7380, has been variously proposed tobe a Be star, a D-type symbiotic and a Herbig Ae/Be star in separate studies.Here we present optical spectroscopy, near-IR photometry and narrow bandH-alpha imaging of the nebulosity in its environment. Analysis of all theseresults, including the spectral energy distribution constructed from availabledata, strongly indicate the source to be a Herbig Ae/Be star. The star is foundto be accompanied by a nebulosity with an interesting structure. A bow shockshaped structure, similar to a cometary nebula, is seen very close to the starwith its apex oriented towards the photoionizing source of this region (i.e.the star DH Cep). An interesting spectroscopic finding, from the forbidden[SII] 6716, 6731 \AA and [OI] 6300 \AA lines, is the detection of ablue-shifted high velocity outflow (200 +/- 50 km/s) from the star.

Studies of a possible new Herbig Ae/Be star in the open cluster NGC 7380