A VLA 3.6 centimeter survey of N-type carbon starsLUTTERMOSER, D. G; BROWN, A.The Astrophysical journal. 1992, Vol 384, Num 2, pp 634-639, issn 0004-637X, p.1Article

Stochastic shock waves as a candidate mechanism for the formation of the He I λ10830 line in cool giant starsCUNTZ, M; LUTTERMOSER, D. G.The Astrophysical journal. 1990, Vol 353, Num 2, pp L39-L43, issn 0004-637X, 2Article

Ultraviolet spectra and chromospheres of cool carbon starsJOHNSON, H. R; LUTTERMOSER, D. G.The Astrophysical journal. 1987, Vol 314, Num 1, pp 329-340, issn 0004-637X, 1Article

Ionization and excitation in cool giant stars. I: Hydrogen and heliumLUTTERMOSER, D. G; JOHNSON, H. R.The Astrophysical journal. 1992, Vol 388, Num 2, pp 579-594, issn 0004-637X, p.1Article

The violet and ultraviolet opacity problem for carbon starsJOHNSON, H. R; LUTTERMOSER, D. G; FAULKNER, D. R et al.The Astrophysical journal. 1988, Vol 332, Num 1, pp 421-431, issn 0004-637X, 1Article

Hydrogen-deficient atmospheres for cool carbon starsJOHNSON, H. R; ALEXANDER, D. R; BOWER, C. D et al.The Astrophysical journal. 1985, Vol 292, Num 1, pp 228-230, issn 0004-637XArticle

Line profile variations in M giants: clues to mass-loss and chromospheric heating mechanismsJUDGE, P. G; LUTTERMOSER, D. G; NEFF, D. H et al.The Astronomical journal (New York). 1993, Vol 105, Num 5, pp 1973-1986, issn 0004-6256Article