SOLAR MODELS, HELIUM CONTENT AND MIXING LENGTHMAZZITELLI I.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 79; NO 1-2; PP. 251-253; BIBL. 16 REF.Article

LUMINOSITY AND MASS FUNCTIONS FOR LOW MAINSEQUENCE STARSMAZZITELLI I.1972; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1972; VOL. 17; NO 2; PP. 378-389; BIBL. 5REF.Serial Issue

WHITE DWARF EXTERNAL LAYERS. IV: INTERPRETATION OF SPECTRAD'ANTONA F; MAZZITELLI I.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 74; NO 2; PP. 161-171; BIBL. 80 REF.Article

INFLUENCE OF THE ATMOSPHERIC COMPOSITION ON THE STRUCTURE OF A WHITE DWARF OF 45 MOD'ANTONA F; MAZZITELLI I.1975; MEM. SOC. ASTR. ITAL.; ITA; DA. 1975; VOL. 46; NO 2; PP. 271-275; ABS. ITA; BIBL. 11 REF.Article

A theoretical relation between the initial mass in main sequence and final white dwarf massMAZZITELLI, I.Memorie della Societa Astronomica Italiana. 1987, Vol 58, Num 1, pp 117-121, issn 0037-8720Conference Paper

EARLY PRE-MAIN-SEQUENCE EVOLUTION WITH DEUTERIUM BURNINGMAZZITELLI I; MORETTI M.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 235; NO 3 PART. 1; PP. 955-959; BIBL. 19 REF.Article

WHITE DWARF EXTERNAL LAYERS. III. ACCRETION AND RELATED PROBLEMS.D'ANTONA F; MAZZITELLI I.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 44; NO 2; PP. 253-257; BIBL. 21 REF.Article

THE PROGENITOR MASSES AND THE LUMINOSITY FUNCTION OF WHITE DWARFS.D'ANTONA F; MAZZITELLI I.1978; ASTR. AND ASTROPHYS.; GERM.; DA. 1978; VOL. 66; NO 3; PP. 453-461; BIBL. 41 REF.Article

COOLING SEQUENCE OF A PURE HELIUM WHITE DWARF OF 0.15 SOLAR MASSESD'ANTONA F; MAGNI G; MAZZITELLI I et al.1972; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1972; VOL. 19; NO 1; PP. 151-158; ABS. ITAL.; BIBL. 10 REF.Serial Issue

CHEMICAL AND PHYSICAL PROPERTIES OF NEARBY POPULATION I STARS.CARDINI D; MAZZITELLI I; ROSSI L et al.1977; ASTROPHYS. SPACE SCI.; NLD; DA. 1977; VOL. 48; NO 2; PP. 283-292; BIBL. 6 REF.Article

The relation between initial and minimum final white dwarf mass for population I starsMAZZITELLI, I; D'ANTONA, F.The Astrophysical journal. 1986, Vol 311, Num 2, pp 762-773, issn 0004-637X, 1Article

Mass-luminosity relation and initial mass function at the faint end of the main sequence. Is there a real deficit of very low mass stars?D'ANTONA, F; MAZZITELLI, I.Astronomy and astrophysics (Berlin. Print). 1983, Vol 127, Num 1, pp 149-152, issn 0004-6361Article

"PHOTOMETRY AND ANALYSIS OF THE SHORT PERIOD VARIABILITY OF THE NOVA CYGNI 1975".MARCOCCI M; MAZZITELLI I; MESSI R et al.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 55; NO 2; PP. 171-175; BIBL. 11 REF.Article

Horizontal branch evolutionCALOI, V; MAZZITELLI, I.Astronomy and astrophysics (Berlin. Print). 1993, Vol 271, Num 1, pp 139-148, issn 0004-6361Article

The relation between initial and minimum final white dwarf mass for population I starsMAZZITELLI, I; D'ANTONA, F.The Astrophysical journal. 1986, Vol 311, Num 2, pp 762-773, issn 0004-637X, 1Article

Cooling of White DwarfsD'ANTONA, F; MAZZITELLI, I.Annual review of astronomy and astrophysics. 1990, Vol 28, pp 139-181, issn 0066-4146, 43 p.Article

Evolution from the main sequence to the white dwarf stage for a 3 M_○. starMAZZITELLI, I; D'ANTONA, F.The Astrophysical journal. 1986, Vol 308, Num 2, pp 706-720, issn 0004-637X, 1Article

AN EVOLUTIONARY UPPER LIMIT FOR THE EFFECTIVE TEMPERATURES OF HORIZONTAL-BRANCH STARS AND THE OCCURRENCE OF GAPS IN THEIR OBSERVED DISTRIBUTIONCAPUTO F; CHIEFFI A; MAZZITELLI I et al.1981; ASTROPHYSICAL PARAMETERS FOR GLOBULAR CLUSTERS. INTERNATIONAL ASTRONOMICAL UNION. COLLOQUIUM. 68/1981-10-07/NEW YORK NY; USA; SCHENECTADY NY: L. DAVIS PRESS; DA. 1981; PP. 313-317; BIBL. 4 REF.Conference Paper

The turn-on of mass transfer in cataclysmic binariesD'ANTONA, F; MAZZITELLI, I; RITTER, H et al.Astronomy and astrophysics (Berlin. Print). 1989, Vol 225, Num 2, pp 391-404, issn 0004-6361Article

Observational constraints to the theory of Planetary nebulae evolutionD'ANTONA, F; MAZZITELLI, I; SABBADIN, F et al.Astrophysics and space science library. 1987, Vol 135, pp 121-130, issn 0067-0057Conference Paper

Helioseismological test of a new model for stellar convectionPATERNO, L; VENTURA, R; CANUTO, V. M et al.The Astrophysical journal. 1993, Vol 402, Num 2, pp 733-740, issn 0004-637X, 1Article

85 Peg A : what age for a low-metallicity solar-like star?D'ANTONA, F; CARDINI, D; DI MAURO, M. P et al.Monthly Notices of the Royal Astronomical Society. 2005, Vol 363, Num 3, pp 847-856, issn 0035-8711, 10 p.Article