Other
Scientific paper
Nov 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apjs...44..383s&link_type=abstract
Astrophysical Journal Supplement Series, vol. 44, Nov. 1980, p. 383-402.
Other
82
Chromosphere, Cool Stars, H Lines, K Lines, Late Stars, Spectral Energy Distribution, Stellar Atmospheres, Stellar Spectra, High Resolution, Iue, Stellar Envelopes, Stellar Luminosity, Stellar Temperature, Ultraviolet Spectra, Velocity Distribution
Scientific paper
We present high-resolution lUE spectra of the emission cores of the Mg II resonance doublet at 280 nm in a selection of 54 stars covering a range of spectral type from F8 to MS and of luminosity class from supergiant (Ia) to subgiant (IV). These spectra were obtained with the LWR echelle system onboard the IUE satellite, and have been calibrated in absolute flux units using OAO 2 photometry of Eta UMa as a standard, plus the Barnes and Evans relations for stellar angular diameters. The uncertainty in flux is probably of order 20%. We discuss the qualitative line profile groupings, as determined by Basri and Linsky, and derive chromospheric radiative losses in the h and k lines; we discuss these loss rates as functions of effective temperature and luminosity class. We make further comparisons of these rates with rates derived for the Ca II H and K lines by Linsky and his colleagues. Chromospheric velocity fields and indicators of circumstellar envelopes are discussed in terms of profile asymmetries and other diagnostics. Line width measures and velocity shifts of the central reversals are tabulated, among other quantities, and several correlations noted. Finally, we discuss the relation of the Wilson K index and stellar coronae to Mg II emission, and note the occurrence of Fe II emission lines in the middle range of the UV of late-type stars.
Basri Gibor S.
Linsky Jeffrey L.
Mullan Dermott J.
Stencel Robert E.
Worden Simon P.
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