Evolutionary tracks and isochrones for low-and intermediate-mass stars: From 0.15 to 7, and from to 0.03 L Girardi, A Bressan, G Bertelli, C Chiosi Astronomy and Astrophysics Supplement Series 141 (3), 371-383, 2000 | 3166 | 2000 |
Theoretical isochrones from models with new radiative opacities G Bertelli, A Bressan, C Chiosi, F Fagotto, E Nasi Astronomy and Astrophysics Suppl., Vol. 106, p. 275-302 (1994) 106, 275-302, 1994 | 2121 | 1994 |
Theoretical isochrones in several photometric systems-I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets L Girardi, G Bertelli, A Bressan, C Chiosi, MAT Groenewegen, P Marigo, ... Astronomy & Astrophysics 391 (1), 195-212, 2002 | 1443 | 2002 |
Evolutionary sequences of stellar models with new radiative opacities. II-Z= 0.02 A Bressan, F Fagotto, G Bertelli, C Chiosi Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 100, no …, 1993 | 926 | 1993 |
The evolution of massive stars with mass loss C Chiosi, A Maeder IN: Annual review of astronomy and astrophysics. Volume 24 (A87-26730 10-90 …, 1986 | 838 | 1986 |
Galactic chemical enrichment with new metallicity dependent stellar yields L Portinari, C Chiosi, A Bressan Astronomy and Astrophysics, v. 334, p. 505-539 (1998) 334, 505-539, 1998 | 639 | 1998 |
Spectrophotometric evolution of elliptical galaxies. 1: Ultraviolet excess and color-magnitude-redshift relations A Bressan, C Chiosi, F Fagotto The Astrophysical Journal Supplement Series, vol. 94, no. 1, p. 63-115 94 …, 1994 | 607 | 1994 |
Evolutionary sequences of stellar models with new radiative opacities. IV. Z= 0.004 and Z= 0.008 F Fagotto, A Bressan, G Bertelli, C Chiosi Astronomy and Astrophysics Suppl., Vol. 105, p. 29-38 (1994) 105, 29-38, 1994 | 569 | 1994 |
Evolutionary sequences of stellar models with new radiative opacities. III. Z= 0.0004 and Z= 0.05 F Fagotto, A Bressan, G Bertelli, C Chiosi Astronomy and Astrophysics Suppl., Vol. 104, p. 365-376 (1994) 104, 365-376, 1994 | 543 | 1994 |
The initial mass function for massive stars CD Garmany, PS Conti, C Chiosi Astrophysical Journal, Part 1, vol. 263, Dec. 15, 1982, p. 777-790. Research …, 1982 | 432 | 1982 |
Massive stars evolution with mass-loss. I-20-100-solar-mass models C Chiosi, E Nasi, SR Sreenivasan Astronomy and Astrophysics, vol. 63, no. 1-2, Feb. 1978, p. 103-124 …, 1978 | 424* | 1978 |
Mass loss and overshooting in massive stars AG Bressan, C Chiosi, G Bertelli Astronomy and Astrophysics, vol. 102, no. 1, Sept. 1981, p. 25-30. Consiglio …, 1981 | 378 | 1981 |
Evolutionary sequences of stellar models with new radiative opacities. VI. L Girardi, A Bressan, C Chiosi, G Bertelli, E Nasi Astronomy and Astrophysics Supplement Series 117 (1), 113-125, 1996 | 352 | 1996 |
Evolutionary tracks and isochrones for alpha-enhanced stars B Salasnich, L Girardi, A Weiss, C Chiosi arXiv preprint astro-ph/0007388, 2000 | 351 | 2000 |
Evolutionary sequences of stellar models with semiconvection and convective overshoot. I-Z= 0.008 M Alongi, G Bertelli, A Bressan, C Chiosi, F Fagotto, L Greggio, E Nasi Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no …, 1993 | 344 | 1993 |
Zero-metallicity stars-I. Evolution at constant mass P Marigo, L Girardi, C Chiosi, PR Wood Astronomy & Astrophysics 371 (1), 152-173, 2001 | 328 | 2001 |
Theoretical isochrones in several photometric systems-II. The Sloan Digital Sky Survey ugriz system L Girardi, EK Grebel, M Odenkirchen, C Chiosi Astronomy & Astrophysics 422 (1), 205-215, 2004 | 315 | 2004 |
New developments in understanding the HR diagram C Chiosi, G Bertelli, A Bressan In: Annual review of astronomy and astrophysics. Vol. 30 (A93-25826 09-90 …, 1992 | 315 | 1992 |
Age distribution of LMC clusters from their integrated UBV colors: history of star formation LA Girardi, C Chiosi, G Bertelli, A Bressan Astronomy and Astrophysics. Berlin. Vol. 298, no. 1 (June 1995), p. 87-106, 1995 | 301 | 1995 |
The TP-AGB phase: a new model P Marigo, A Bressan, C Chiosi Astronomy & Astrophysics 313, 545-565, 1996 | 278 | 1996 |