RT Journal Article
T1 Analysis of the far ultraviolet emission lines in late type stars
A1 Castro Rubio, Elisa De
A1 Fernández Figueroa, María José
A1 Rego Fernández, Manuel
A1 Ponz, D.
AB Far ultraviolet emission lines in a sample of seven stars of spectral type later than F5 and different luminosity class have been analyzed to calculate the electron density and pressure in the formation region of the lines. Three different methods were used. We obtain electron pressures larger than solar for all dwarf stars of the sample. The low resolution observations were made with the IUE satellite.
PB EDP Sciencies
SN 0004-6361
YR 1981
FD 1981
LK https://hdl.handle.net/20.500.14352/64993
UL https://hdl.handle.net/20.500.14352/64993
LA eng
NO © European Southern Observatory
DS Docta Complutense
RD 9 abr 2025