Silicates do nucleate in oxygen-rich circumstellar outflows : New vapor pressure data for SiONUTH, Joseph A; FERGUSON, Frank T.The Astrophysical journal. 2006, Vol 649, Num 2, pp 1178-1183, issn 0004-637X, 6 p., 1Article

Radio photosphere and mass-loss envelope of VY canis majorisLIPSCY, S. J; JURA, M; REID, M. J et al.The Astrophysical journal. 2005, Vol 626, Num 1, pp 439-445, issn 0004-637X, 7 p., 1Article

PROPER MOTIONS OF H₂O MASERS IN THE WATER FOUNTAIN SOURCE IRAS 19190+1102DAY, F. M; PIHLSTRÖM, Y. M; CLAUSSEN, M. J et al.The Astrophysical journal. 2010, Vol 713, Num 2, pp 986-991, issn 0004-637X, 6 p., 1Article

Classical thermal evaporation of clouds: an electrostatic analogyBALBUS, S. A.The Astrophysical journal. 1985, Vol 291, Num 2, pp 518-522, issn 0004-637X, part 1Article

Some comments on empirical fits to stellar mass loss ratesVARDYA, M. S.The Astrophysical journal. 1987, Vol 312, Num 2, issn 0004-637X, 812, 1Article

Nouvelle évidence pour la perte de masse dans les céphéides classiquesSTIFT, M. J.Astronomy and astrophysics (Berlin. Print). 1984, Vol 140, Num 2, pp 445-448, issn 0004-6361Article

Atmospheric corrosion in MauritiusSURNAM, B. Y. R; OLETI, C. V.Corrosion engineering, science and technology. 2012, Vol 47, Num 6, pp 446-455, issn 1478-422X, 10 p.Article

Durabilidad del aluminio desnudo y anodizado en atmÓsferas de muy diferentes corrosividades. II. Aluminio anodizado = Durability of bare and anodised aluminium in atmosphere of very different corrosivities. II. Anodised aluminiumLOPEZ, V; ESCUDERO, E; GONZALEZ, J. A et al.Revista de metalurgia (Madrid). 2004, Vol 40, Num 4, pp 270-279, issn 0034-8570, 10 p.Article

Optical signatures of circumstellar interaction in type IIP supernovaeCHUGAI, Nikolai N; CHEVALIER, Roger A; UTROBIN, Victor P et al.The Astrophysical journal. 2007, Vol 662, Num 2, pp 1136-1147, issn 0004-637X, 12 p., 1Article

ON THE BINDING ENERGY PARAMETER λ OF COMMON ENVELOPE EVOLUTIONXU, Xiao-Jie; LI, Xiang-Dong.The Astrophysical journal. 2010, Vol 716, Num 1, pp 114-121, issn 0004-637X, 8 p., 1Article

Carbon, nitrogen, and oxygen galactic gradients : A solution to the carbon enrichment problemCARIGI, Leticia; PEIMBERT, Manuel; ESTEBAN, César et al.The Astrophysical journal. 2005, Vol 623, Num 1, pp 213-224, issn 0004-637X, 12 p., 1Article

Moderate asphericity of the SN 2002ic circumstellar envelopeCHUGAI, Nikolai N; CHEVALIER, Roger A.The Astrophysical journal. 2007, Vol 657, Num 1, pp 378-382, issn 0004-637X, 5 p., 1Article

On the flaring of jet-sustaining accretion disksNAMOUNI, Fathi.The Astrophysical journal. 2007, Vol 659, Num 2, pp 1505-1510, issn 0004-637X, 6 p., 1Article

Cleaning up η Carinae : Detection of ammonia in the homunculus nebulaSMITH, Nathan; BROOKS, Kate J; KORIBALSKI, Bärbel S et al.The Astrophysical journal. 2006, Vol 645, Num 1, issn 0004-637X, L41-L44, 2Article

Size distribution of collisionally evolved asteroidal populations: analytical solution for self-similar collision cascadesWILLIAMS, D. R; WETHERILL, G. W.Icarus (New York, NY). 1994, Vol 107, Num 1, pp 117-128, issn 0019-1035Article

On bipolar ejectionCAMERON, A. G. W.The Astrophysical journal. 1985, Vol 299, Num 2, pp L83-L86, issn 0004-637XArticle

Vibrational instability of Wolf-Rayet starsMAEDER, A.Astronomy and astrophysics (Berlin. Print). 1985, Vol 147, Num 2, pp 300-308, issn 0004-6361Article

Supergiant variability: theoretical pulsation periods and comparison with observationsLOVY, D; MAEDER, A; NOELS, A et al.Astronomy and astrophysics (Berlin. Print). 1984, Vol 133, Num 2, pp 307-312, issn 0004-6361Article

Yes, you can control lost and unaccounted for gasPipeline & gas journal. 1984, Vol 211, Num 6, pp 22-28, issn 0032-0188Article

Semianalytical treatment of the hydrodynamics of supernova remnants during the snowplow phaseGAFFET, B.The Astrophysical journal. 1983, Vol 273, Num 1, pp 267-279, issn 0004-637XArticle

Recent mass loss episode of the Be star ο AndGHOSH, K. K; JAYKUMAR, K; ROSARIO, M. J et al.Information bulletin on variable stars. 1986, Num 2897, issn 0374-0676, 4 p.Serial Issue

Mass loss rates from protostars and 01(63 μm) shock luminositiesHOLLENBACH, D.Icarus (New York, NY). 1985, Vol 61, Num 1, pp 36-39, issn 0019-1035Article

The stability of stellar structure in non-equilibrium thermodynamics. III. The PPI reaction allowing for mass lossWANG ZHEN-YI; PENG QIU-HE; HUANG KE-LIANG et al.Chinese astronomy and astrophysics. 1984, Vol 8, Num 3, pp 223-227, issn 0275-1062Article

Cooking of pre-sliced meat = La cuisson de la viande prédécoupéeBURFOOT, D; SWAIN, M. J; JAMES, S. J et al.Journal of Food Technology. 1985, Vol 20, Num 2, pp 155-161, issn 0022-1163Article

Peculiar thermal behavior of diallyl oxalate prepolymerYAMAWAKI, M; MATSUMOTO, A; OIWA, M et al.Journal of applied polymer science. 1984, Vol 29, Num 5, pp 1761-1769, issn 0021-8995Article