TY  - JOUR
A1  - Steinke, M.
A1  - Oskinova, Lida
A1  - Hamann, Wolf-Rainer
A1  - Sander, A.
T1  - The Wolf-Rayet stars WR102c and 102ka and their isolation
T2  - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
N2  - While the majority of very massive stars is clearly found in clusters, there are also very massive objects not associated with any cluster, suggesting they may have been born in isolation. In order to gain more insights, we studied the regions around two WR stars in the Galactic Center region. To understand the nature of the potential cluster around massive stars, photometry alone is not sufficient. We therefore used the ESO VLT/SINFONI integral field spectrograph to obtain photometry and spectra for the whole region around our two candidate stars. In total, more than 60 stars have been found and assigned a spectral type.
Y1  - 2015
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/8850
UR  - https://nbn-resolving.org/urn:nbn:de:kobv:517-opus4-88503
SP  - 365
ER  -