Unveiling the birth and evolution of the HII region Sh2-173

S. CICHOWOLSKI; GISELA ROMERO; M.E. ORTEGA; C.E. CAPPA; J. VASQUEZ

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

WILEY-BLACKWELL PUBLISHING, INC

Año: 2009 vol. 394 p. 900 - 915

0035-8711

Based on a multiwavelength study, the interstellar medium around the H II region Sh2-173 has been analyzed. The ionized region is clearly detected in the optical and in the radio continuum images. The analysis of the H I data shows a region of low emissivity that hasan excellent morphological correlation with the radio continuum emission. The H II region is partially bordered by a photodissociation region, which, in turn, is encircled by a molecular structure. The H I and CO structures related to Sh2-173 are observed in the velocity ranges from –25 to –31kms−1, and from –27 to –39 kms−1, respectively. Taking into account the presence of noncircular motions in the Perseus spiral arm, together with previous distance estimates for the region, we adopt a distance of 2.5 ± 0.5 kpc for Sh2-173. Seven hot stars were identified in the field of Sh2-173, being only one an O-type star. The amount of energetic photons emitted by this star is enough to keep the region ionized and heat the dust. Given that an expanding H II region may trigger star formation, a search for YSO candidates was made using different infrared point source catalogues. A population of 46 YSO candidateswas identified projected onto the molecular clouds.On the other hand, Sh2-173 is located in a dense edge of a large ( 5◦) H I shell, GSH117.8+1.5-35. The possibility for Sh2-173 of being part of a hierarchical system of three generations is suggested. In this scenario, the large H I shell, which was probably originateddue to the action of CasOB5, would have triggered the formation of Sh2-173, which, in turn, is triggering new stars in its surrounding molecular cloud. To test this hypothesis, the ages of both, the H II region and the large shell, were estimated and compared. We concluded that Sh2-173 is a young H II region of about 0.6 - 1.0 Myr old. As for the large shell we obtained a dynamical age of 5 ± 1 Myr. These age estimates, together with the relative location ofdifferent structures, support the hypothesis that Sh2-173 is part of a hierarchical system.