THE INFLUENCE OF MASS LOSS ON THE EVOLUTION OF BINARIESDE LOORE C.1981; ASTROPHYS. SPACE SCI. LIBR.; ISSN 0067-0057; NLD; DA. 1981; VOL. 89; PP. 405-430; BIBL. 2 P.Conference Paper

THE EVOLUTION OF MASSIVE STARSDE LOORE C.1980; SPACE SCI. REV.; NLD; DA. 1980; VOL. 26; NO 2; PP. 113-155; BIBL. 4 P.Article

LINE IDENTIFICATION LIST OF 3 HYA.HENSBERGE H; DE LOORE C.1975; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1975; VOL. 20; NO 2; PP. 183-197; BIBL. 31 REF.Article

HEATING OF THE SOLAR TRANSITION ZONE AND CORONA.VANBEVEREN D; DE LOORE C.1976; SOLAR PHYS.; NETHERL.; DA. 1976; VOL. 50; NO 1; PP. 99-108; BIBL. 40 REF.Article

DETERMINATION OF ABUNDANCES AND THE SURFACE MAGNETIC FIELD STRENGTH OF 3 HYA BY A CURVE OF GROWTH METHOD.HENSBERGE H; DE LOORE C.1974; ASTR. AND ASTROPHYS.; GERM.; DA. 1974; VOL. 37; NO 2; PP. 367-373; BIBL. 69 REF.Article

Comparative study of evolutionary tracks of massive starsDE LOORE, C.Astronomy and astrophysics (Berlin. Print). 1988, Vol 203, Num 1, pp 71-78, issn 0004-6361Article

MASSES AND MASS LOSS FROM O AND OF STARSLAMERS HJGLM; PAERELS FBS; DE LOORE C et al.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 87; NO 1-2; PP. 68-76; BIBL. 40 REF.Article

EVOLUTION OF MASSIVE CLOSE BINARIES. IV. EVOLUTION OF A 10M _CERCLE.+8M _CERCLE. SYSTEM INTO A SYSTEM WITH A WHITE DWARF COMPONENT.DE GREVE JP; DE LOORE C.1976; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1976; VOL. 43; NO 1; PP. 35-46; BIBL. 22 REF.Article

TWO TYPES OF EVOLUTION OF MASSIVE CLOSE BINARY SYSTEMS.DE LOORE C; DE GREVE JP.1976; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1976; NO 73; PP. 27-34; BIBL. 30 REF.; (STRUCT. EVOL. CLOSE BINARY SYST. SYMP.; CAMBRIDGE, ENGL.; 1975)Conference Paper

Stellar and galactic windsDE LOORE, C.Physica scripta. T. 1984, Vol 7, pp 25-33, issn 0281-1847Article

THE EFFECT OF MASS LOSS ON THE AGE-DETERMINATION OF YOUNG CLUSTERS, WITH AN APPLICATION TO THE ORION OB-ASSOCIATIONPAERELS FBS; LAMERS HJGLM; DE LOORE C et al.1980; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1980; VOL. 90; NO 1-2; PP. 204-206; BIBL. 18 REF.Article

PERIOD CHANGES IN BINARY SYSTEMS DURING THE WOLF-RAYET STAGE.DE GREVE JP; DE LOORE C.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 42; NO 1; PP. 91-94; BIBL. 18 REF.Article

EVOLUTION OF MASSIVE CLOSE BINARIES. I. THE X-RAY BINARY STAGE.DE LOORE C; DE GREVE JP.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 35; NO 2; PP. 241-247; BIBL. 14 REF.Article

Observations of binaries and evolutionary implicationsDE LOORE, C.Astrophysics and space science. 1984, Vol 99, Num 1-2, pp 199-227, issn 0004-640XArticle

Evolutionary sequences for massive close binaries with galactic abundances with Rogers-Iglesias opacitiesDE LOORE, C; VANBEVEREN, D.Astronomy & astrophysics. Supplement Series (Print). 1994, Vol 105, Num 1, pp 21-28, issn 0365-0138Article

Late stages of the evolution of close binariesDE LOORE, C; SUTANTYO, W.Astrophysics and space science. 1984, Vol 99, Num 1-2, pp 335-354, issn 0004-640XArticle

PHOTOMETRY OF PECULIAR A STARS.HENSBERGE H; DE LOORE C; ZUIDERWIJK EJ et al.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 48; NO 3; PP. 383-387; BIBL. 24 REF.Article

MASS LOSS FROM ALPHA CYG (A2 IA) DERIVED FROM THE PROFILES OF LOW EXCITATION FE_II LINESHENSBERGE H; LAMERS HJGLM; DE LOORE C et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 106; NO 1; PP. 137-150; BIBL. 22 REF.Article

EVOLUTION OF MASSIVE CLOSE BINARIES. II. THE POST X-RAY BINARY STAGE: ORIGIN OF RUN-AWAY AND BINARY PULSARS.DE LOORE C; DE GREVE JP; DE CUYPER JP et al.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 36; NO 1; PP. 219-225; BIBL. 17 REF.Article

The evolution of WR+O binaries into massive X-ray binariesHELLINGS, P; DE LOORE, C.Astronomy and astrophysics (Berlin. Print). 1986, Vol 161, Num 1, pp 75-84, issn 0004-6361Article

THE EFFECT OF STELLAR EVOLUTION ON THE SYNDHRONOUS ROTATION OF COMPONENTS OF MASSIVE CLOSE BINARIESSUTANTYO W; DE GREVE JP; DE LOORE C et al.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 83; NO 1-2; PP. 252-255; BIBL. 12 REF.Article

PARAMETERS OF MASSIVE STARS FOR MAIN SEQUENCE EVOLUTION WITHOUT AND WITH STELLAR WINDDE LOORE C; DE GREVE JP; VANBEVEREN D et al.1978; ASTR. AND ASTROPHYS., SUPPL. SER.; DEU; DA. 1978; VOL. 34; NO 3; PP. 363-368; BIBL. 16 REF.Article

A DETAILED STUDY OF THE SPECTRUM OF THE BINARY X-RAY SOURCE HD 153919 (3U 1700-37). I. RADIAL VELOCITY DATA IN THE BLUE SPECTRAL REGION.HAMMERSCHLAG HENSBERGE G; DE LOORE C; VAN DEN HEUVEL EPJ et al.1978; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1978; VOL. 32; NO 3; PP. 375-377; BIBL. 3 REF.Article

Evolutionary sequences for massive close binary stars with Magellanic Cloud metallicities with Rogers-Iglesias opacitiesDE LOORE, C; VANBEVEREN, D.Astronomy & astrophysics. Supplement Series (Print). 1994, Vol 103, Num 1, pp 67-82, issn 0365-0138Article

A binary evolutionary model for the progenitor of SN 1987 ADE LOORE, C; VANBEVEREN, D.Astronomy and astrophysics (Berlin. Print). 1992, Vol 260, Num 1-2, pp 273-282, issn 0004-6361Article