D. Garmany i P. Massey, Pub. Astron. Soc. Pacific 93, 500-503 (1981). The initial mass function for massive stars, C. D. Garmany, P. S. Conti i C. Chiosi, Ap. J. 263, 777-790 (1982). Sk-71 34: A new Wolf-Rayet star in the Large Magellanic Cloud, P. S. Conti i C. D. Garmany, Publ. Astron. Soc. Pacific 92, 411-412 (1983). The evolution of massive stars: The numbers and distribution of O stars and Wolf-Rayet stars, P. S. Conti, C. D. Garmany, C. de Loore i D. Vanbeveren, Ap. J. 274, 302-312 (1983). Absolute spectrophotometry of Wolf-Rayet stars from 1200 to 7000: A cautionary tale, C. D. Garmany, P. Massey i P. S. Conti, Ap. J. 278, 233-240 (1984). Mass loss in O-type stars: Parameters which affect it, C. D. Garmany i P. S. Conti, Ap. J. 284, 705-711 (1984). O-Stars in the Galaxy, C. D. Garmany, Publ. Astron. Soc. Pacific 96, 779 (1984). Stellar winds from hot stars in the Magellanic Clouds, C. D. Garmany i P. S. Conti, Ap. J. 293, 407-413 (1985). Extreme Be stars in the Magellanic Clouds, C. D. Garmany i R. M. Humphreys, Astron. J. 90, 2009-2014 (1985). HR 4049: The hottest proto-planetary nebula star or a run-away hypergiant at high galactic latitude surrounded by a dust cloud?, H. J. G. L. M. Lamers, L. B. F. M. Waters, C. D. Garmany, M. R. Perez i C. Waelkens, Astron. Astrophys.