Content About: Peter Conti
The stellar content of 30 doradus derived from spatially integrated ultraviolet spectra: A test of spectral synthesis models
Published: 10/19/2012 - 11:07am Type of Content: People - Faculty & Research Groups
Mid-infrared diagnostics of metal-rich H ii regions from VLT and Spitzer spectroscopy of young massive stars in W31
Hubble Space Telescope Ultraviolet Spectroscopy of NGC 1741: A Nearby Template for Distant Energetic Starbursts
The spectra of Wolf-Rayet stars. I - Optical line strengths and the hydrogen-to-helium ratios in WN type 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
Ultraviolet spectroscopic variability of the WN 5 star HD 50896: timescales and linear physical dimensions of the perturbations
Spectroscopic studies of O-type stars. VII. Rotational velocities V*sin(i) and evidence for macroturbulent motions.
Connection between nonradial pulsations and stellar winds in massive stars. V - Stellar winds and variability in hot luminous stars
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.