The VIIth catalogue of galactic Wolf–Rayet stars
KA Van Der Hucht - New Astronomy Reviews, 2001 - Elsevier
The VIIth catalogue of galactic PopulationI Wolf–Rayet stars provides improved coordinates,
spectral types and bv photometry of known WR stars and adds 71 new WR stars to the …
spectral types and bv photometry of known WR stars and adds 71 new WR stars to the …
Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters
T Nugis, H Lamers - Astronomy and Astrophysics, Vol. 360, p …, 2000 - adsabs.harvard.edu
Clumping-corrected mass-loss rates of 64 Galactic Wolf-Rayet (WR) stars are used to study
the dependence of mass-loss rates, momentum transfer efficiencies and terminal velocities …
the dependence of mass-loss rates, momentum transfer efficiencies and terminal velocities …
Clumping-corrected mass-loss rates of Wolf-Rayet stars
T Nugis, PA Crowther, AJ Willis - … , v. 333, p. 956-969 (1998), 1998 - adsabs.harvard.edu
Mass-loss rates of Galactic Wolf-Rayet stars have been determined from their radio emission
power and spectral index (alpha= dln {f_ν}/dln ν), accounting for the clumped structure and …
power and spectral index (alpha= dln {f_ν}/dln ν), accounting for the clumped structure and …
On the role of the WNH phase in the evolution of very massive stars: enabling the LBV instability with feedback
N Smith, PS Conti - The Astrophysical Journal, 2008 - iopscience.iop.org
We propose the new designation “WNH” for luminous Wolf-Rayet (WR) stars of the nitrogen
sequence with hydrogen in their spectra. These have been commonly referred to as WNL …
sequence with hydrogen in their spectra. These have been commonly referred to as WNL …
Photometric Determination of Orbital Inclinations and Mass Loss Rates for Wolf-Rayet Stars in WR+ O Binaries
R Lamontagne, AFJ Moffat, L Drissen… - … Journal v. 112, p …, 1996 - adsabs.harvard.edu
We analyze the atmospheric" eclipse" light curves of all 13 short-period (P< 30 d) Galactic
binary WR+ O systems with solved orbits, excluding the 3 known photospheric eclipsers …
binary WR+ O systems with solved orbits, excluding the 3 known photospheric eclipsers …
A 2.3 day periodic variability in the apparently single Wolf-Rayet star WR 134: Collapsed companion or rotational modulation?
T Morel, SV Marchenko, PRJ Eenens… - The Astrophysical …, 1999 - iopscience.iop.org
The apparently single WN 6 type star WR 134 (HD 191765) is distinguished among the Wolf-
Rayet star population by its strong, presumably cyclical (𝒫 ≈ 2.3 day) spectral …
Rayet star population by its strong, presumably cyclical (𝒫 ≈ 2.3 day) spectral …
X-rays from colliding stellar winds: the case of close Wolf–Rayet+ O binary systems
SA Zhekov - Monthly Notices of the Royal Astronomical Society, 2012 - academic.oup.com
We have analysed the X-ray emission from a sample of close Wolf–Rayet+ O (WR+ O)
binaries using data from the public Chandra and XMM–Newton archives. Global spectral fits …
binaries using data from the public Chandra and XMM–Newton archives. Global spectral fits …
The OB association LH 58 in the Large Magellanic Cloud
CD Garmany, P Massey… - … Journal, vol. 108, no. 4, p …, 1994 - adsabs.harvard.edu
We present CCD photometry and spectroscopy for stars in Lucke-Hodge 58, an isolated OB
association in the Large Magellanic Cloud (LMC) northwest of 30 Doradus. The photometric …
association in the Large Magellanic Cloud (LMC) northwest of 30 Doradus. The photometric …
Wolf-Rayet stars and relativistic objects: Distinctions between the mass distributions in close binary systems
AM Cherepashchuk - Astronomy Reports, 2001 - Springer
The observed properties of Wolf-Rayet stars and relativistic objects in close binary systems
are analyzed. The final masses M CO f for the carbon-oxygen cores of WR stars in WR+ O …
are analyzed. The final masses M CO f for the carbon-oxygen cores of WR stars in WR+ O …
Close Binary Stars. VI: New Research Methods
AM Cherepashchuk - Astronomy Reports, 2022 - Springer
A review of new methods for studying close binary systems (CBSs) is presented. Methods for
determining the masses of relativistic objects (X-ray pulsars, black holes, radio pulsars) in …
determining the masses of relativistic objects (X-ray pulsars, black holes, radio pulsars) in …