Content About: Peter Conti
Spectroscopic studies of O-type stars. VII. Rotational velocities V*sin(i) and evidence for macroturbulent motions.
Hubble Space Telescope Ultraviolet Spectroscopy of NGC 1741: A Nearby Template for Distant Energetic Starbursts
Connection between nonradial pulsations and stellar winds in massive stars. V - Stellar winds and variability in hot luminous stars
Infrared Spectra of Massive Stars in Transition: WNL, Of, Of/WN, Be, B[e], and Luminous Blue Variable Stars
Studies of massive stars in the Magellanic Clouds. II - New spectral classification of OB stars in the SMC
Spectroscopic studies of Wolf-Rayet stars with absorption lines. II - The WN8 standard star HD 177230
Ultraviolet spectroscopic variability of the WN 5 star HD 50896: timescales and linear physical dimensions of the perturbations
Spectroscopic studies of Wolf-Rayet stars. IV - Optical spectrophotometry of the emission lines in galactic and large Magellanic Cloud stars
Joint Institute for Laboratory Astrophysics of the National Bureau of Standards and the University of Colorado, Boulder, Colorado. Observatory report.
Massive star formation and feedback in W49A: the source of our Galaxy's most luminous water maser outflow
Spectroscopic studies of Wolf-Rayet stars with absorption lines. IV - The mass of CX Cephei /WN5+O/. V - HD 9974, a single WN3