TY  - CHAP
AU  - Gómez De Castro, Ana Inés
AU  - Pagano, Isabella
AU  - Linsky, Jeff
PY  - 2005
SN  - 92-9092-871-9
UR  - https://hdl.handle.net/20.500.14352/53142
AB  - To progress in our understanding of cool stars is instrumental to have access to UV (mid-high resolution) spectroscopy. In fact, the UV range supplies a richness of experimental data which is unmatched by any other spectral domain for the study of...
LA  - eng
M2  - 155
PB  - European Space Agency
KW  - Hubble-space-telescope
KW  - Coronal forbidden lines
KW  - Star au microscopii
KW  - Mass-loss rates
KW  - Echelle spectra
KW  - Alpha-centauri
KW  - Ab doradus
KW  - Flares
KW  - Stars : atmospheres
KW  - Stars : formation
KW  - UV spectroscopy
TI  - The relevance and future of the ultraviolet range
TY  - book part
ER  -