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ON THE CONSTANCY OF THE ABSOLUTE MAGNITUDE MB(15) OF A CLASSICAL NOVA 15 DAYS AFTER MAXIMUM LIGHTSHARA MM.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 243; NO 1; PART. 1; PP. 268-270; BIBL. 11 REF.Article

A THEORETICAL EXPLANATION OF THE ABSOLUTE MAGNITUDE-DECLINE TIME (MBETA -T3) RELATIONSHIP FOR CLASSICAL NOVAESHARA MM.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 243; NO 3; PART. 1; PP. 926-934; BIBL. 32 REF.Article

WHITE DWARF-MAIN SEQUENCE STAR COLLISIONS.SHARA MM; SHAVIV G.1977; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1977; VOL. 179; NO 3; PP. 705-718; BIBL. 21 REF.Article

THE FLOW OF AN INFINITE COMPRESSIBLE FLUID PAST A RIGID, GRAVITATING SPHERE AND INTERACTING DEGENERATE STAR-RED GIANT BINARIESSHARA MM; SHAVIV G.1980; ASTROPHYS. SPACE SCI.; NLD; DA. 1980; VOL. 67; NO 2; PP. 427-443; BIBL. 19 REF.Article

HYDRODYNAMIC SIMULATIONS OF WHITE-DWARF-MAIN-SEQUENCE STAR COLLISIONS.SHARA MM; SHAVIV G.1978; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1978; VOL. 183; NO 3; PP. 687-700; BIBL. 16 REF.Article

EVOLUTION OF DENSE GALACTIC NUCLEI THORUGH DWARF STAR COLLISIONS.SHARA MM; SHAVIV G.1974; NATURE; G.B.; DA. 1974; VOL. 248; NO 5447; PP. 398-400; BIBL. 15 REF.Article

THE RECOVERY OF CK VULPECULAE (NOVA 1670) - THE OLDEST "OLD NOVA"SHARA MM; MOFFAT AFJ.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 258; NO 1; PP. L41-L44; BIBL. 10 REF.Article

X-RAY INTENSITIES FROM THE FLOW OF A STELLAR WIND PAST A COMPACT OBJECTLIVIO M; SHARA MM; SHAVIV G et al.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 233; NO 2 PART. 1; PP. 704-710; BIBL. 31 REF.Article

NON-EJECTING NOVAE AS EUV SOURCES.SHARA MM; PRIALNIK D; SHAVIV G et al.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 61; NO 3; PP. 363-367; BIBL. 28 REF.Article

WHAT DETERMINES THE SPEED CLASS OF NOVAE.SHARA MM; PRIALNIK D; SHAVIV G et al.1980; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1980; VOL. 239; NO 2; PART. 1; PP. 586-591; BIBL. 31 REF.Article

THE EVOLUTION OF A FAST NOVA MODEL WITH A 3=0.03 ENVELOPE FROM PRE-EXPLOSION TO DECLINEPRIALNIK D; SHARA MM; SHAVIV G et al.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 72; NO 1-2; PP. 192-203; BIBL. 24 REF.Article

THE EVOLUTION OF A SLOW NOVA MODEL WITH AZ=0.03 ENVELOPE FROM PRE-EXPLOSION TO EXTINCTION.PRIALNIK D; SHARA MM; SHAVIV G et al.1978; ASTR. AND ASTROPHYS.; GERM.; DA. 1978; VOL. 62; NO 3; PP. 339-348; BIBL. 39 REF.Article

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