Showing 1–14 of 14 results
/ Date/ Name
Jan 11, 2009Highly Accelerated Diamagnetic Plasmoids: A New X-ray Production Mechanism for OB Stellar WindsJan 25, 2010The Importance of XUV Radiation as a Solution to the P V Mass Loss Rate Discrepancy in O-StarsJun 29, 2007An Extensive Collection of Stellar Wind X-ray Source Region Emission Line Parameters,Temperatures, Velocities, and Their Radial Distributions as Obtained from Chandra Observations of 17 OB StarsApr 29, 2015A Coordinated X-ray and Optical Campaign of the Nearest Massive Eclipsing Binary, delta Orionis Aa: III. Analysis of Optical Photometric MOST and Spectroscopic (Ground Based) VariationsMar 15, 2020A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the $ζ\,$Puppis WindJul 11, 2017The variability of the BRITE-est Wolf-Rayet binary, $γ^2$ Velorum I. Photometric and spectroscopic evidence for colliding windsAug 3, 2012On the Weak-Wind Problem in Massive Stars: X-ray Spectra Reveal a Massive Hot Wind in μ ColumbaeOct 23, 2017BRITE-Constellation high-precision time-dependent photometry of the early-O-type supergiant $ζ$ Puppis unveils the photospheric drivers of its small- and large-scale wind structuresFeb 23, 2011An Introduction to the Chandra Carina Complex ProjectDec 8, 2000Chandra Discovers a Very High Density X-ray Plasma on the O-Star Zeta OrionisJul 27, 2009The Correlation between X-Ray Line Ionization and Optical Spectral Types of the OB StarsMay 28, 2004Chandra Observations of Associates of $η$ Car: II. SpectraDec 4, 2007X-Atlas: An Online Archive of Chandra's Stellar High Energy Transmission Gratings ObservationsNov 13, 2020Correlated X-ray and optical variability in the O-type supergiant zeta Puppis