SOME INSIGHT INTO GRAVITATIONAL RED-SHIFT: IS ANTIGRAVITY REALLY TO BE RULED OUT.MOLTENI D; ZIINO G.1978; LETTERE NUOVO CIMENTO; ITA; DA. 1978; VOL. 23; NO 13; PP. 487-488; BIBL. 3 REF.Article

DYNAMO ACTION IN A SUPERMASSIVE ROTATOR AND THE ACTIVE GALACTIC NUCLEIBELVEDERE G; MOLTENI D.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 263; NO 2; PART. 1; PP. 611-614; BIBL. 38 REF.Article

HIGH X-RAY LUMINOSITY FROM DYNAMO STARSBELVEDERE G; MOLTENI D.1981; SPACE SCI. REV.; ISSN 0038-6308; NLD; DA. 1981; VOL. 30; NO 1-4; PP. 181-184; BIBL. 8 REF.Conference Paper

STELLAR DYNAMO AND THE GALACTIC X-RAY SOURCESBELVEDERE G; MOLTENI D.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 102; NO 3; PP. 283-286; BIBL. 19 REF.Article

EVIDENCE OF A CONTINUOUS CHANGE IN THE PERIOD OF CYGNUS X-3MANZO G; MOLTENI D; ROBBA NR et al.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 70; NO 1-2; PP. 317-318; BIBL. 9 REF.Article

Smoothed particle hydrodynamics confronts theory : formation of standing shocks in accretion disks and winds around black holesCHAKRABARTI, S. K; MOLTENI, D.The Astrophysical journal. 1993, Vol 417, Num 2, pp 671-676, issn 0004-637X, 1Article

The role of hard binaries in cluster evolutionGIANNONE, G; MOLTENI, D.Symposium - International astronomical union. 1985, Num 113, issn 0074-1809, 321Conference Paper

The role of initial binaries in cluster evolution: direct N-body calculationsGIANNONE, G; MOLTENI, D.Astronomy and astrophysics (Berlin. Print). 1985, Vol 143, Num 2, pp 321-326, issn 0004-6361Article

Magnetic field in a supermassive rotator as an energy source for active galactic nucleiBELVEDERE, G; MOLTENI, D.Physica scripta. T. 1984, Vol 7, pp 163-164, issn 0281-1847Article

Transport phenomena in magmas and in astrophysical clusters = Phénomènes de transport dans les magmas et dans les systèmes stellairesLUCIDO, G; MOLTENI, D.Mineralogica et petrographica acta. 1985, Vol 29, pp 1-12, issn 0540-1437Article

ON THE SPIN DOWN EPISODES OF VELA X-1MOLTENI D; RAPISARDA M; RE S et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 111; NO 2; PP. 365-367; BIBL. 14 REF.Article

The X-ray structure of Centaurus a from 0.1 to 50 keV observations with EXOSATMORINI, M; ANSELMO, F; MOLTENI, D et al.The Astrophysical journal. 1989, Vol 347, Num 2, pp 750-759, issn 0004-637X, 1Article

The jets and disc of SS 433 at super-Eddington luminositiesOKUDA, T; LIPUNOVA, G. V; MOLTENI, D et al.Monthly notices of the Royal Astronomical Society (Print). 2009, Vol 398, Num 4, pp 1668-1677, issn 0035-8711, 10 p.Article

Shock oscillation model for quasi-periodic oscillations in stellar mass and supermassive black holesOKUDA, T; TERESI, V; MOLTENI, D et al.Monthly Notices of the Royal Astronomical Society. 2007, Vol 377, Num 4, pp 1431-1438, issn 0035-8711, 8 p.Article

Performance of MIMO-OFDMA Systems in Correlated Fading Channels and Non-Stationary InterferenceMOLTENI, D; NICOLI, M; SPAGNOLINI, U et al.IEEE transactions on wireless communications. 2011, Vol 10, Num 5, pp 1480-1494, issn 1536-1276, 15 p.Article

Linking air-sea energy exchanges and European anchovy potential spawning groundGRAMMAUTA, R; MOLTENI, D; CUTTITTA, A et al.The European physical journal. B, Condensed matter physics. 2008, Vol 65, Num 3, pp 459-467, issn 1434-6028, 9 p.Conference Paper

SPH simulations of Shakura-Sunyaev instability at intermediate accretion ratesTERESI, V; MOLTENI, D; TOSCANO, E et al.Monthly Notices of the Royal Astronomical Society. 2004, Vol 348, Num 1, pp 361-367, issn 0035-8711, 7 p.Article

The X-ray spectrum of Markarian 509 observed by ExosatMORINI, M; LIPANI, N. A; MOLTENI, D et al.The Astrophysical journal. 1987, Vol 317, Num 1, pp 145-151, issn 0004-637X, 1Article

A simple model of radiative emission in M87VITANZA, E; TERESI, V; MOLTENI, D et al.The Astrophysical journal. 2006, Vol 643, Num 1, pp 222-225, issn 0004-637X, 4 p., 1Article

Black hole accretion discs and jets at super-Eddington luminosityOKUDA, T; TERESI, V; TOSCANO, E et al.Monthly Notices of the Royal Astronomical Society. 2005, Vol 357, Num 1, pp 295-303, issn 0035-8711, 9 p.Article

Ab initio simulations of accretion disc instabilityTERESI, V; MOLTENI, D; TOSCANO, E et al.Monthly Notices of the Royal Astronomical Society. 2004, Vol 351, Num 1, pp 297-310, issn 0035-8711, 14 p.Article

A three-dimensional smoothed particle hydrodynamics simulation of the active phase of SS Cyg-type discs and its implications for the mass transfer burst modelLANZAFAME, G; BELVEDERE, G; MOLTENI, D et al.Monthly Notices of the Royal Astronomical Society. 1993, Vol 263, Num 4, pp 839-850, issn 0035-8711Article

The role of the secondary's rotation in disc formation and structure: an SPH three-dimensional analysisBELVEDERE, G; LANZAFAME, G; MOLTENI, D et al.Astronomy and astrophysics (Berlin. Print). 1993, Vol 280, Num 2, pp 525-535, issn 0004-6361Article

3D simulations of the SS Cyg accretion disc in the quiescent phaseLANZAFAME, G; BELVEDERE, G; MOLTENI, D et al.Monthly Notices of the Royal Astronomical Society. 1992, Vol 258, Num 1, pp 152-158, issn 0035-8711Article

An exceptional change in the X-ray flux and spectrum of the Seyfert 1 galaxy E 1615+061PIRO, L; MASSARO, E; PEROLA, G. C et al.The Astrophysical journal. 1988, Vol 325, Num 2, pp L25-L28, issn 0004-637X, part 2Article