au.\*:("MILGROM M")
Results 1 to 25 of 85
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REVIEW OF THE THEORIES ON SS 433MILGROM M.1981; VISTAS ASTRON.; ISSN 0083-6656; GBR; DA. 1981; VOL. 25; NO 1-2; PP. 141-151; BIBL. 37 REF.Conference Paper
SS433: THE ACCELERATION AND COLLIMATION MECHANISMSMILGROM M.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 78; NO 1; PP. L9-L12; BIBL. 12 REF.Article
THOMSON SCATTERED LINES IN THE SPECTRUM OF SS 433. A POWERFUL TOOL FOR STUDYING THE SYSTEMMILGROM M.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 78; NO 3; PP. L17-L20; BIBL. 14 REF.Article
SPECTROSCOPIC PROPERTIES OF HZ HERCULIS IN MODEL CALCULATIONS.MILGROM M.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 206; NO 3 PART. 1; PP. 869-875; BIBL. 36 REF.Article
CALCULATION OF THE OPTICAL APPEARANCE OF CYG X-2.MILGROM M.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 50; NO 2; PP. 273-277; BIBL. 24 REF.Article
ON THE NATURE OF THE GALACTIC BULGE X-RAY SOURCES.MILGROM M.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 67; NO 3; PP. L25-L28; BIBL. 42 REF.Article
ON THE ORIGIN OF OPTICAL EMISSION LINES IN SPECTRA OF X-RAY BINARIES.MILGROM M.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 207; NO 3 PART. 1; PP. 902-906; BIBL. 38 REF.Article
THE HEATING EFFECT IN SCORPIUS X-1.MILGROM M.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 208; NO 1, PART. 1; PP. 191-198; BIBL. 30 REF.Article
ANOMALOUS PERIASTRON POSITIONS IN X-RAY BINARIESMILGROM M.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 70; NO 6; PP. 763-767; BIBL. 15 REF.Article
DOES X PERSEI REALLY HAVE A MASSIVE COMPANION.MILGROM M.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 53; NO 2; PP. 321-323; BIBL. 18 REF.Article
The virial theorem for action-governed theoriesMILGROM, M.Physics letters. A. 1994, Vol 190, Num 1, pp 17-21, issn 0375-9601Article
On the use of galaxy rotation curves to test the modified dynamicsMILGROM, M.The Astrophysical journal. 1988, Vol 333, Num 2, pp 689-693, issn 0004-637X, part 1Article
La modification des lois de NewtonMILGROM, M.Recherche (Paris, 1970). 1988, Num 196, pp 182-190, issn 0029-5671Article
A modification of the newtonian dynamics: implications for galaxy systemsMILGROM, M.The Astrophysical journal. 1983, Vol 270, Num 2, pp 384-389, issn 0004-637XArticle
CYGNUS X-3: A COCOONED X-RAY BINARY PULSAR.MILGROM M; PINES D.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 220; NO 1 PART. 1; PP. 272-278; BIBL. 36 REF.Article
MODELS FOR X-RAY ILLUMINATED ATMOSPHERES.MILGROM M; SALPETER EE.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 196; NO 2 PART. 1; PP. 583-588; BIBL. 15 REF.Article
Why is the rapid burster different from all other galactic-bulge X-ray sources?MILGROM, M.Astronomy and astrophysics (Berlin. Print). 1987, Vol 172, Num 1-2, pp L1-L2, issn 0004-6361Article
The light-echo model for luminous arcsMILGROM, M.Astronomy and astrophysics (Berlin. Print). 1987, Vol 182, Num 1, pp L21-L24, issn 0004-6361Article
Isothermal spheres in the modified dynamicsMILGROM, M.The Astrophysical journal. 1984, Vol 287, Num 2, pp 571-576, issn 0004-637X, 1Article
HYDROGEN AND HELIUM LINES IN THEORETICAL MODELS OF SCORPIUS X-1 AND CYGNUS X-2.MILGROM M; KATZ JI.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 205; NO 2 PART. 1; PP. 545-549; BIBL. 17 REF.Article
RESONANCE FORM FACTORS, SCALING, AND REGGE BEHAVIOR IN INELASTIC ELECTRON-NUCLEON SCATTERINGAVNI Y; MILGROM M.1973; PHYS. REV., D; U.S.A.; DA. 1973; VOL. 7; NO 5; PP. 1463-1468; BIBL. 20 REF.Serial Issue
Concerning the preferred surface density of giant molecular clouds in the GalaxyMILGROM, M.Astronomy and astrophysics (Berlin. Print). 1989, Vol 211, Num 1, pp 37-40, issn 0004-6361Article
Can the hidden mass be negative?MILGROM, M.The Astrophysical journal. 1986, Vol 306, Num 1, pp 9-15, issn 0004-637X, 1Article
Solutions for the modified newtonian dynamics field equationMILGROM, M.The Astrophysical journal. 1986, Vol 302, Num 2, pp 617-625, issn 0004-637X, 1Article
OBSERVATIONAL CONSTRAINTS ON THE MASS OF SMC X-1.AVNI Y; MILGROM M.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 212; NO 1 PART. 2; PP. L17-L20; BIBL. 1/2 P.Article