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VARIATIONS ULTRARAPIDES DANS LA RAIE SPECTRALE HALPHA DE L'ETOILE BE PHI PERMAMATKAZINA A KH.1975; ASTR. CIRK., IZDAV. BJURO ASTR. SOOBSHCH. AKAD. NAUK S.S.S.R.; S.S.S.R.; DA. 1975; NO 867; PP. 1-4Article

A TENTATIVE ENVELOPE MODEL OF PHI PERSEI.SUZUKI M.1976; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1976; VOL. 39; NO 2; PP. 495-497; BIBL. 5 REF.Article

WAVELENGTH DEPENDENCE OF POLARIZATION. XXX. INTRINSIC POLARIZATION IN PHI PERSEI.COYNE GV; MCLEAN IS.1975; ASTR. J.; U.S.A.; DA. 1975; VOL. 80; NO 9; PP. 702-710; BIBL. 24 REF.Article

SPECTROPHOTOMETRIE DE LA RAIE HALPHA DE L'ETOILE PHI PERMAMATKAZINA A KH.1978; TRUDY ASTROFIZ. INST., ALMA-ATA; S.S.S.R.; DA. 1978; VOL. 31; PP. 73-79; ABS. ANGL.; BIBL. 5 REF.Article

TOWARD A MODEL FOR THE BE BINARY SYSTEM PHI PER.HENDRY EM.1976; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1976; NO 70; PP. 429-437; BIBL. 15 REF.; (BE AND SHELL STARS. MERRILL-MCLAUGHLIN MEM. SYMP.; BASS RIVER, MASS.; 1975)Conference Paper

A SPECTROSCOPIC STUDY OF THE BINARY BE STAR PHI PERSEIPOECKERT R.1981; PUBL. ASTRON. SOC. PAC.; ISSN 0004-6280; USA; DA. 1981; VOL. 93; NO 553; PP. 297-317; BIBL. 39 REF.Article

ULTRAVIOLET SPECTROSCOPY OF PHI PERSEIKITCHIN CR.1982; MON. NOT. R. ASTRON. SOC.; ISSN 0035-8711; GBR; DA. 1982; VOL. 198; NO 2; PP. 457-472; BIBL. 24 REF.Article

HIGH-RESOLUTION POLARIZATION STRUCTURE OF HBETA IN BE SHELL STARS MEASURED WITH A NEW DIGICON SPECTROPOLARIMETERMCLEAN IS; COYNE GV; FRECKER JE et al.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 228; NO 3 PART. 1; PP. 802-808; BIBL. 18 REF.Article

AN ENVELOPE MODEL OF PHI PERSISUZUKI M.1980; PUBL. ASTRON. SOC. JPN; ISSN 0004-6264; JPN; DA. 1980; VOL. 32; NO 2; PP. 331-340; BIBL. 17 REF.Article

PHOTOELECTRIC PHOTOMETRY OF SOME BO STARSDAPERGOLAS A; DI COLA G; GUARNIERI A et al.1981; INF. BULL. VARIABLE STARS; ISSN 0374-0676; HUN; DA. 1981; NO 1920; 3 P.; BIBL. 6 REF.Serial Issue

POLARIMETRY OF BE STARS AT 1.25 AND 2.2 MICRONSJONES TJ.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 228; NO 3 PART. 1; PP. 787-801; BIBL. 31 REF.Article

FOURIER TRANSFORM SPECTROSCOPY OF FOUR O-B STARS FROM 4800 TO 12000 AJOHNSON HL; WISNIEWSKI WZ; FAY TD et al.1978; REV. MEX. ASTR. ASTROFIS.; MEX; DA. 1978; VOL. 2; NO 4; PP. 273-308; ABS. ESP; BIBL. 37 REF.Article

INTERPRETATION OF EMISSION LINE PROFILES OF ROTATING SHELLSPOELLITSCH GF.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 97; NO 1; PP. 175-181; BIBL. 19 REF.Article

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