Atmospheric parameters of stars for UV models (Koleva+, 2012)
The spectral predictions of stellar population models are not as accurate in the ultra-violet (UV) as in the optical wavelength domain. One of the reasons is the lack of high-quality stellar libraries. The New Generation Stellar Library (NGSL), recently released, represents a significant step towards the improvement of this situation. To prepare
Koleva, M. et al.
Advertised on:
11
2011