TY  - JOUR
A1  - Bestenlehner, J. M.
T1  - Stellar parameters from photometric data for fainter and more distant Wolf-Rayet stars
T2  - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
N2  - Spectroscopy is the preferred way to study the physical and wind properties of Wolf-Rayet (WR) stars, but with decreasing brightness and increasing distance of the object spectroscopy become very expensive. However, photometry still delivers a high signal to noise ratio. Current and past astronomical surveys and space missions provide large data sets, that can be harvested to discover new WR stars and study them over a wide metallicity range with the help of state of the art stellar atmosphere and evolutionary models.
Y1  - 2015
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/8839
UR  - https://nbn-resolving.org/urn:nbn:de:kobv:517-opus4-88390
SP  - 354
ER  -