GeminiFocus January 2015 | Page 13

Figure 4. The sample of eight stars was selected on the basis of Paschen α emission, characteristic of massive stars. Observations using the Gemini Near-Infrared Spectrograph (GNIRS) and Near-infrared Integral Field Spectrometer (NIFS), both on the Gemini North telescope, provide spectroscopy with a resolution of around 50 kilometers per second. Sample stars located near the Arches cluster are similar to the cluster population (in terms of age, mass, and spectral characteristics), suggesting that they were originally cluster members. The massive field stars could have been dynamically ejected from the cluster, especially through three-body interactions. Two examples show velocities that are similar to those of nearby molecular and ionized gas clouds, which implies a physical association with these neighboring star-forming regions. The researchers suggest that one of these in particular, dubbed P35 (Figure 4), may have January 2015 formed at this site. In contrast, other stars show differences in motion compared with nearby gaseous regions, which suggests that the stars are only passing by and were not formed originally at these locations. In addition, the new spectroscopy confirms main sequence masses exceeding 50 MSun in all cases and enables additional spectral classification; Dong et al. also report the identification of a new O If+ star. Complete results appear in Monthly Notices of the Royal Astronomical Society (view here) and a preprint is available here. Upper panels show near-infrared continuum and Paschen α images of target P35 and its associated HII region. The position-velocity plot (c) around the wavelength of Brackett γ is extracted from the GNIRS longslit spectrum (whose location is marked with horizontal lines in the upper panels). Low surface brightness features marked with arrows in (b) are evident in the positionvelocity plot. Nancy A. Levenson is Deputy Director and Head of Science at Gemini Observatory and can be reached at: [email protected] Rachel Mason is an Associate Astronomer at Gemini North. She can be reached at: [email protected] GeminiFocus 11