GAMMA CASSIOPEIAE AND THE TRANSIENT X-RAY SOURCE MX 0053+60.MARLBOROUGH JM.1977; PUBL. ASTR. SOC. PACIF.; U.S.A.; DA. 1977; VOL. 89; NO 528; PP. 122-126; BIBL. 30 REF.Article

ULTRAVIOLET OBSERVATIONS OF BE STARS. I. MACROSCOPIC RADIAL MOTIONS IN THE ATMOSPHERES OF EARLY BE STARS.MARLBOROUGH JM.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 216; NO 2, PART. 1; PP. 446-456; BIBL. 41 REF.Article

MODELS FOR THE CIRCUMSTELLAR ENVELOPES OF BE STARS.MARLBOROUGH JM.1976; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1976; NO 70; PP. 335-370; BIBL. 2 P.; (BE AND SHELL STARS. MERRILL-MCLAUGHLIN MEM. SYMP.; BASS RIVER, MASS.; 1975)Conference Paper

WEBER AND DAVIS REVISITED: MASS LOSING ROTATING MAGNETIC WINDSBARKER PK; MARLBOROUGH JM.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 254; NO 1; PART. 1; PP. 297-300; BIBL. 18 REF.Article

THE EFFECTS OF ELECTRON SCATTERING ON BALMER EMISSION LINES IN BE STARSPOECKERT R; MARLBOROUGH JM.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 233; NO 1 PART. 1; PP. 259-266; BIBL. 18 REF.Article

CIRCULAR AND LINEAR POLARIZATION IN A-TYPE SHELL STARSCLAYTON GC; MARLBOROUGH JM.1980; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1980; VOL. 242; NO 1; PART. 1; PP. 165-170; BIBL. 26 REF.Article

RAPIDLY ROTATING STARS WITH OPTICALLY THIN STELLAR WINDS.MARLBOROUGH JM; ZAMIR M.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 195; NO 1 PART. 1; PP. 145-155; BIBL. 18 REF.Article

THE BALMER PROGRESSION DURING PLEIONE'S SHELL EPISODE, 1938-1954MARLBOROUGH JM; GREDLEY PR.1972; ASTROPHYS. J.,; U.S.A.; DA. 1972; VOL. 178; NO 2PART1; PP. 477-480; BIBL. 8REF.Serial Issue

A REPORT ON SYMPOSIUM NO. 83 OF THE INTERNATIONAL ASTRONOMICAL UNION "MASS LOSS AND EVOLUTION OF O TYPE STARS". I: GENERAL REVIEWCOWLEY AP; MARLBOROUGH JM.1979; EARTH EXTRATERRESTR. SCI.; GBR; DA. 1979; VOL. 3; NO 7-8; PP. 177-182Article

A MODEL FOR GAMMA CASSIOPEIAE.POECKERT R; MARLBOROUGH JM.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 220; NO 3 PART. 1; PP. 940-961; BIBL. 49 REF.Article

LINEAR POLARIZATION OF HALPHA IN THE BE STAR GAMMA CASSIOPEIAE.POECKERT R; MARLBOROUGH JM.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 218; NO 1 PART. 1; PP. 220-226; BIBL. 22 REF.Article

A SURVEY OF MASS LOSS FROM BE AND SHELL STARS USING ULTRAVIOLET DATA FROM COPERNICUS.MARLBOROUGH JM; SNOW TP JR.1976; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1976; NO 70; PP. 179-189; BIBL. 1 P.; (BE AND SHELL STARS. MERRILL-MCLAUGHLIN MEM. SYMP.; BASS RIVER, MASS.; 1975)Conference Paper

OBSERVATIONS OF OMICRON ANDROMEDAE. III: A MODELPOECKERT R; CULLIVER AF; MARLBOROUGH JM et al.1982; PUBL. ASTRON. SOC. PAC.; ISSN 0004-6280; USA; DA. 1982; VOL. 94; NO 557; PP. 87-96; BIBL. 26 REF.Article

ULTRAVIOLET AND OPTICAL SPECTRAL VARIABILITY IN THE BE STAR Y CASSIOPEIAE: A CORONAL MODEL FOR THE EMISSION.MARLBOROUGH JM; SNOW TP JR; SLETTEBAK A et al.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 224; NO 1 PART. 1; PP. 157-166; BIBL. 35 REF.Article

THE MAGNETIC FIELD OF ZETA PUPPISBARKER PK; LANDSTREET JD; MARLBOROUGH JM et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 250; NO 1; PART. 1; PP. 300-305; BIBL. 27 REF.Article

TT ARIETIS: AN EVOLVED, VERY SHORT PERIOD BINARY.COWLEY AP; CRAMPTON D; HUTCHINGS JB et al.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 195; NO 2 PART. 1; PP. 413-421; BIBL. 18 REF.Article