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au.\*:("AUGASON GC")

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THEORETICAL PROFILES FOR THE 1-0 S(1)H2 LINE IN CARBON STARSGOORVITCH D; GOEBEL JH; AUGASON GC et al.1980; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1980; VOL. 240; NO 2; PART. 1; PP. 588-596; BIBL. 28 REF.Article

COMPARISON OF PREDICTED AND OBSERVED SPECTRAL ENERGY DISTRIBUTION OF K AND M STARS. I: ALPHA BOOTISAUGASON GC; TAYLOR BJ; STRECKER DW et al.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 235; NO 1 PART. 1; PP. 138-145; BIBL. 44 REF.Article

WATER VAPOR ABSORPTION SPECTRA OF THE UPPER ATMOSPHERE (45-185 CM-1).AUGASON GC; MORD AJ; WITTEBORN FC et al.1975; APPL. OPT.; U.S.A.; DA. 1975; VOL. 14; NO 9; PP. 2146-2150; BIBL. 34 REF.Article

SPECTRUM OF THE KLEINMANN-LOW NEBULA FROM 29 TO 125 MICROMETERS.ERICKSON EF; STRECKER DW; SIMPSON JP et al.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 212; NO 3 PART. 1; PP. 696-703; BIBL. 29 REF.Article

AIRCRAFT OBSERVATIONS OF VENUS'NEAR-INFRARED REFLECTION SPECTRUM: IMPLICATIONS FOR CLOUD COMPOSITION.POLLACK JB; ERICKSON EF; WITTEBORN FC et al.1974; ICARUS; U.S.A.; DA. 1974; VOL. 23; NO 1; PP. 8-26; BIBL. 1 P. 1/2Article

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