MULTIPOLE ANISOTROPY OF THE COSMIC BACKGROUND RADIATION IN DENSITY WAVE MODELSFABBRI R; GUIDI I; NATALE V et al.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 257; NO 1; PART. 1; PP. 17-22; BIBL. 16 REF.Article

INFRARED EMISSION FROM DUST IN STELLAR AGGREGATESAIELLO S; GUIDI I; MENCARAGLIA F et al.1978; MEM. SOC. ASTR. ITAL.; ITA; DA. 1978; VOL. 49; NO 1; PP. 271-280; BIBL. 20 REF.Conference Paper

LARGE-SCALE ANISOTROPY OF THE 3 K BACKGROUND RADIATION IN DENSITY WAVE MODELSFABBRI R; GUIDI I; NATALE V et al.1983; ASTRONOMY AND ASTROPHYSICS; ISSN 0004-6361; DEU; DA. 1983; VOL. 122; NO 1-2; PP. 151-163; BIBL. 19 REF.Article

IS GAS IN THE ORION NEBULA DEPLETED.AIELLO S; GUIDI I; PERINOTTO M et al.1978; ASTROPHYS. SPACE SCI.; NLD; DA. 1978; VOL. 54; NO 2; PP. 417-423; BIBL. 27 REF.Article

SULLA DEPLEZIONE GASSOSA NELLA NEBULOSA DI ORIONEAIELLO S; GUIDI I; PERINOTTO M et al.1977; MEM. SOC. ASTR. ITAL.; ITA; DA. 1977; VOL. 48; NO 4; PP. 751-757; ABS. ENG; BIBL. 18 REF.Article

THE SHAPE OF THE POWER SPECTRUM OF COSMIC RAY AT GROUND LEVEL UP TO 7 X 10^-3 HZ.ATTOLINI MR; CECCHINI S; GUIDI I et al.1975; PLANET. SPACE SCI.; G.B.; DA. 1975; VOL. 23; NO 12; PP. 1603-1609; BIBL. 10 REF.Article

LIMITATIONS OF GROUND BASED NEAR AND FAR INFRARED ASTRONOMY.DALL'OGLIO G; GUIDI I; MELCHIORRI B et al.1975; INFRARED PHYS.; G.B.; DA. 1975; VOL. 15; NO 1; PP. 13-17; BIBL. 6 REF.Article

POWER SPECTRUM ANALYSIS OF COSMIC-RAY FLUCTUATIONS. II. THE MEASUREMENTS ERROR EFFECT.ATTOLINI MR; CECCHINI S; GUIDI I et al.1974; LETTERE NUOVO CIMENTO; ITAL.; DA. 1974; VOL. 11; NO 7; PP. 386-390; BIBL. 7 REF.Article

A MICHELSON INTERFEROMETER FOR ASTRONOMICAL APPLICATIONSGUIDI I; MELCHIORRI B; MELCHIORRI F et al.1978; INFRARED PHYS.; GBR; DA. 1978; VOL. 18; NO 4; PP. 267-273; BIBL. 16 REF.Article

ULTRAVIOLET EXTINCTION TOWARDS FAR OB ASSOCIATIONSAIELLO S; BARSELLA B; GUIDI I et al.1982; ASTROPHYSICS AND SPACE SCIENCE; ISSN 0004-640X; NLD; DA. 1982; VOL. 87; NO 1-2; PP. 463-476; BIBL. 2 P.Article

POWER SPECTRUM ANALYSIS OF COSMIC-RAY FLUCTUATIONS. III. THE POWER SPECTRAL DENSITY IN THE REGION (10^-7 DIV. ENT 10^-4) HZ.ATTOLINI MR; CECCHINI S; GUIDI I et al.1974; LETTERE NUOVO CIMENTO; ITAL.; DA. 1974; VOL. 11; NO 7; PP. 391-399; BIBL. 11 REF.Article

INTERSTELLAR EXTINCTION ON THE SGR OB-5 ASSOCIATIONAIELLO S; BARSELLA B; BONETTI A et al.1979; MEM. SOC. ASTR. ITAL.; ITA; DA. 1979; VOL. 50; NO 2; PP. 195-196; BIBL. 7 REF.Conference Paper

FAR INFRARED BACKGROUND ASTRONOMY AT GROUND.DALL'OGLIO G; FONTI S; GUIDI I et al.1975; NUOVO CIMENTO; ITAL.; DA. 1975; VOL. 27; NO 1; PP. 27-40; ABS. ITAL. RUSSE; BIBL. 29 REF.Article

CO Abundances in the Magellanic CloudsBEL, N; VIALA, Y. P; GUIDI, I et al.Nuovo cimento della società italiana di fisica. C. 1985, Vol 8, Num 3, pp 243-247, issn 0390-5551Article

Chemical equilibrium from diffuse to dense clouds. II: Interstellar clouds in the Magellanic cloudsBEL, N; VIALA, Y. P; GUIDI, I et al.Astronomy and astrophysics (Berlin. Print). 1986, Vol 160, Num 2, pp 301-309, issn 0004-6361Article

Search for extragalactic backgrounds: a balloon-borne 4-band FIR differential photometer with large throughputMASI, S; DALL'OGLIO, G; GUIDI, I et al.Astronomy and astrophysics (Berlin. Print). 1989, Vol 226, Num 1, pp 357-365, issn 0004-6361Article