au.\*:("HEIDMANN N")
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A SCHEME OF ATMOSPHERIC REGIONS. III: CHROMOSPHERES OF EMISSION-LINE STARS. 1: FORMATION OF HALPHA EMISSION LINE CORES IN T TAURI-TYPE STARSHEIDMANN N; THOMAS RN.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 87; NO 1-2; PP. 36-54; BIBL. 55 REF.Article
OPTICAL POSITIONS OF BRIGHT GALAXIES. III.GALLOUET L; HEIDMANN N; DAMPIERRE F et al.1975; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1975; VOL. 19; NO 1; PP. 1-19; BIBL. 6 REF.Article
FORMATION OF PERMITTED LINES IN THE SPECTRUM OF TYPE 1 SEYFERT GALAXIES AND QUASARS: FE II LINES, PRELIMINARY DISCUSSIONCOLLIN SOUFFRIN S; JOLY M; HEIDMANN N et al.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 72; NO 3; PP. 293-308; BIBL. 53 REF.Article
FORMATION OF PERMITTED LINES IN THE SPECTRUM OF TYPE 1 SEYFERT GALAXIES AND QUASARS. II: FE II LINES AND THE LOW EXCITATION REGIONCOLLIN SOUFFRIN S; DUMONT S; HEIDMANN N et al.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 83; NO 1-2; PP. 190-198; BIBL. 37 REF.Article
THE ABUNDANCE DETERMINATION IN A STELLAR ATMOSPHERE 1. LTE EXPERIMENTATION USING AN ARTIFICIAL NON-LTE SPECTRUM.DUMONT S; HEIDMANN N; JEFFERIES JT et al.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 40; NO 1-2; PP. 127-132; BIBL. 28 REF.Article