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Results 1 to 25 of 48

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INTERPRETATION OF THE LINE PROFILES OF THE 8 MICRON BAND OF SILICON MONOXIDE FROM VY CANIS MAJORISVAN BLERKOM D; XINJIE M.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 252; NO 2; PART. 2; PP. L73-L74; BIBL. 4 REF.Article

DUST IN THE REFLECTION NEBULA SURROUNDING VY CANIS MAJORIS.JURA M.1975; ASTR. J.; U.S.A.; DA. 1975; VOL. 80; NO 3; PP. 227-231; BIBL. 29 REF.Article

FIRST CELESTIAL WATER VAPOR SOURCES OBSERVED AT ITAPETINGA RADIO OBSERVATORY, BRAZIL.KAUFMANN P; FOGARTY WG; SCALISE E JR et al.1974; ASTR. J.; U.S.A.; DA. 1974; VOL. 79; NO 9; PP. 933-937; BIBL. 11 REF.Article

DETECTION DE LA DIFFERENCE DE POLARISATION DANS LES BANDES MOLECULAIRES ET LE CONTINUUM DANS LES SPECTRES DES VARIABLES ROUGES DE LUMINOSITE ELEVEEDERVIZ TE; DOMBROVSKIJ VA.1973; UCHEN. ZAP. LENINGRAD. GOS. UNIV., MAT. NAUK; S.S.S.R.; DA. 1973; VOL. 29; NO 48; PP. 65-71; ABS. ANGL.; BIBL. 6 REF.Serial Issue

LANGMUIR SCATTERING AND HIGH VELOCITY FEATURES IN STELLAR WATER MASERSCOHEN NL; HOHLFELD RG; GORENSTEIN MV et al.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 95; NO 2; PP. 386-387; BIBL. 10 REF.Article

POLARIZATIONS OF THE INFRARED STARS AND THE GALACTIC CENTRE IN NEAR INFRAREDMAIHARA T; OKUDA H; SATO S et al.1972; MEM. SOC. R. SCI. LIEGE, 8O; )BELG.; DA. 1972; VOL. 3; PP. 417-424; BIBL. 29REF.Serial Issue

A geometrical model of VY Canis Majoris for SiO maser linesZHOU ZHEN-PU; KAIFU, N.Astronomy and astrophysics (Berlin. Print). 1984, Vol 138, Num 2, pp 359-364, issn 0004-6361Article

ON THE NATURE OF MASER SOURCES IN INFRARED STARS.BURDJUZHA VV; RUZMAIKINA TV.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 40; NO 3; PP. 233-236; BIBL. 37 REF.Article

UPPER LIMITS TO THE DIAMETER OF VY CANIS MAJORISBENSAMMAR S; KANDEL R; ASSUS P et al.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 70; NO 4; PP. 585-587; BIBL. 12 REF.Article

Two polarigenic mechanisms in the VY Canis Majoris systemSCHWARZ, H. E; ASPIN, C.Astronomy and astrophysics (Berlin. Print). 1986, Vol 162, Num 1-2, pp 99-102, issn 0004-6361Article

Polarization structure and variability in the optical spectrum of VY Canis MajorisASPIN, C; SCHWARZ, H. E; MCLEAN, I. S et al.Astronomy and astrophysics (Berlin. Print). 1985, Vol 151, Num 1, pp 169-173, issn 0004-6361Article

VLBI OBSERVATIONS OF THE MAIN LINE OH MASERS IN VY CANIS MAJORISBENSON JM; MUTEL RL.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 253; NO 1; PART. 1; PP. 199-207; BIBL. 36 REF.Article

NEW INTERFEROMETRIC POSITIONS OF WATER VAPOR SOURCES.BAUDRY A; FORSTER JR; WELCH WJ et al.1974; ASTR. AND ASTROPHYS.; GERM.; DA. 1974; VOL. 36; NO 2; PP. 217-224; BIBL. 51 REF.Article

MULTIBARELINE VLBI OBSERVATIONS OF THE 1612 MHZ OH MASERS TOWARD NML CYGNI AND VY CANIS MAJORISBENSON JM; MUTEL RL.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 233; NO 1 PART. 1; PP. 119-126; BIBL. 18 REF.Article

SPATIAL HETERODYNE INTERFEROMETRY OF VY CANIS MAJORIS, ALPHA ORIONIS, ALPHA SCORPII, AND R LEONIS AT 11 MICRONSSUTTON EC; STOREY JWV; BETZ AL et al.1977; ASTROPHYS. J.; USA; DA. 1977; VOL. 217; NO 2 PART. 2; PP. L97-L100; BIBL. 24 REF.Article

TiO molecular emission in the spectrum of VY Canis MajorisPHILLIPS, J. G; DAVIS, S. P.Publications of the Astronomical Society of the Pacific. 1987, Vol 99, Num 618, pp 839-841, issn 0004-6280Article

Collisional pumping of SiO masers in evolved starsMIYOSHI, M; MATSUMOTO, K; KAMENO, S et al.Nature (London). 1994, Vol 371, Num 6496, pp 395-397, issn 0028-0836Article

SIO ISOTOPIC MASER EMISSION FROM VY CANIS MAJORISDEGUCHI S; GOOD J; FAN Y et al.1983; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1983; VOL. 264; NO 2; PP. L65-L68; BIBL. 14 REF.Article

TIME VARIATIONS OF STELLAR WATER MASERSCOX GG; PARKER EA.1979; MONTH. NOT. R. ASTR. SOC.; GBR; DA. 1979; VOL. 186; NO 1; PP. 197-215; BIBL. 31 REF.Article

CIRCULAR POLARIZATION OF ZODIACAL LIGHT AND STELLAR RADIATION SCATTERED ON CIRCUMSTELLAR CLOUDSDOLGINOV AZ; MYTROPHANOV IG.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 69; NO 3; PP. 421-430; BIBL. 26 REF.Article

CO OBSERVATIONS OF A MOLECULAR CLOUD COMPLEX ASSOCIATED WITH THE BRIGHT RIM NEAR VY CANIS MAJORIS.LADA CJ; REID MJ.1978; ASTROPHYS. J.; U.S.A.; DA. 1978; VOL. 219; NO 1 PART. 1; PP. 95-104; BIBL. 32 REF.Article

AN INTERPRETATION OF THE APPARENT ORBIT OF VY CMA AB: THE ROTATING HOLEY DUST CLOUD HYPOTHESISWALLERSTEIN G.1978; OBSERVATORY; GBR; DA. 1978; VOL. 98; NO 1026; PP. 224-227; BIBL. 14 REF.Article

RADIATIVE TRANSFER IN GRAY CIRCUMSTELLAR DUST ENVELOPES: VY CANIS MAJORIS REVISITED.SCHWARTZ RD.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 196; NO 3 PART. 1; PP. 745-751; BIBL. 27 REF.Article

MONTE CARLO STUDY OF HIGHLY POLARIZED COOL STARSDANIEL JY.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 111; NO 1; PP. 58-70; BIBL. 1 P.Article

A SIMPLE ESTIMATE OF THE EFFECT OF A THICK CIRCUMSTELLAR DUST SHELL ON PHOTOSPHERIC LINE PROFILESVAN BLERKOM D; CASTOR JI.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 227; NO 2 PART. 1; PP. 543-547; BIBL. 8 REF.Article

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