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Results:
1-16
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Results: 16
Authors:
Mazzei, P
Curir, A
Citation: P. Mazzei et A. Curir, Star formation onset in baryonic disks: The role of a triaxial halo, ASTRON ASTR, 372(3), 2001, pp. 803-819
Authors:
Roussel, H
Sauvage, M
Vigroux, L
Bosma, A
Bonoli, C
Gallais, P
Hawarden, T
Madden, S
Mazzei, P
Citation: H. Roussel et al., The impact of bars on the mid-infrared dust emission of spiral galaxies: global and circumnuclear properties, ASTRON ASTR, 372(2), 2001, pp. 406-426
Authors:
Mazzei, P
Aussel, H
Xu, C
Salvo, M
De Zotti, G
Franceschini, A
Citation: P. Mazzei et al., ISOCAM observations of the deep IRAS 60 micron sample in the NEP region - II. Comparison of ISO and IRAS galaxy counts, NEW ASTRON, 6(5), 2001, pp. 265-276
Authors:
Curir, A
Mazzei, P
Citation: A. Curir et P. Mazzei, The a/m ratio of the baryonic matter and the black holes demography in galaxies, NEW ASTRON, 6(4), 2001, pp. 239-248
Authors:
Roussel, H
Vigroux, L
Bosma, A
Sauvage, M
Bonoli, C
Gallais, P
Hawarden, T
Lequeux, J
Madden, S
Mazzei, P
Citation: H. Roussel et al., An atlas of mid-infrared dust emission in spiral galaxies, ASTRON ASTR, 369(2), 2001, pp. 473-509
Authors:
Barbaro, G
Mazzei, P
Morbidelli, L
Patriarchi, P
Perinotto, M
Citation: G. Barbaro et al., Classification and properties of UV extinction curves, ASTRON ASTR, 365(2), 2001, pp. 157-164
Authors:
Aussel, H
Coia, D
Mazzei, P
De Zotti, G
Franceschini, A
Citation: H. Aussel et al., ISOCAM observations of the very deep IRAS 60 micron sample in the NEP region - I. The data, ASTR AST SS, 141(2), 2000, pp. 257-283
Authors:
Bellia, L
Mazzei, P
Minichiello, F
Palombo, A
Citation: L. Bellia et al., Outdoor-air design conditions relating to the capacity of air-conditioningsystems, INT J ENERG, 24(2), 2000, pp. 121-135
Authors:
Bellia, L
Mazzei, P
Minichiello, F
Palombo, A
Citation: L. Bellia et al., Cooling energy consumption and operating costs: evaporative all-air and air-and-water systems in the Italian climate, INT J ENERG, 24(2), 2000, pp. 163-175
Authors:
Curir, A
Mazzei, P
Citation: A. Curir et P. Mazzei, The influence of a live halo on the bar instability, ASTRO SP SC, 272(1-3), 2000, pp. 45-52
Authors:
Curir, A
Massaglia, S
Mazzei, P
Trussoni, E
Citation: A. Curir et al., Evolution of the interstellar gas in elliptical galaxies, ASTRO SP SC, 272(1-3), 2000, pp. 91-94
Authors:
Mobasher, B
Mazzei, P
Citation: B. Mobasher et P. Mazzei, The effect of dust on photometric redshift measurement: a self-consistent technique, ASTRON ASTR, 363(2), 2000, pp. 517-525
Authors:
Mazzei, P
Palombo, A
Citation: P. Mazzei et A. Palombo, Economic evaluation of hybrid evaporative technology implementation in Italy, BLDG ENVIR, 34(5), 1999, pp. 571-582
Authors:
Curir, A
Mazzei, P
Citation: A. Curir et P. Mazzei, Bar instabilities in disk galaxies: the role of the triaxial halo, ASTRON ASTR, 352(1), 1999, pp. 103-111
Authors:
Curir, A
Mazzei, P
Citation: A. Curir et P. Mazzei, SPH simulations of galaxy evolution including chemo-photometric predictions, NEW ASTRON, 4(1), 1998, pp. 1-20
Authors:
Bellia, L
Mazzei, P
Palombo, A
Citation: L. Bellia et al., Weather data for building energy cost-benefit analysis, INT J ENERG, 22(14), 1998, pp. 1205-1215
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