An XMM-Newton observation of the massive binary HD 159176
M De Becker, G Rauw, JM Pittard, II Antokhin… - Astronomy & …, 2004 - aanda.org
We report the analysis of an XMM-Newton observation of the close binary HD 159176 (O7
V+ O7 V). The observed/ratio reveals an X-ray luminosity exceeding by a factor~ 7 the …
V+ O7 V). The observed/ratio reveals an X-ray luminosity exceeding by a factor~ 7 the …
Resonant Ion Radiation Scattering and the Integrated Atomic Cross-Section as applied to Binary Star Shock Fronts
RJ Pfeiffer - arXiv preprint arXiv:2403.14549, 2024 - arxiv.org
The current literature is rather vague regarding how to calculate the exact numerical value of
the resonant ion scattering cross-section that should be used for a specific bandpass of finite …
the resonant ion scattering cross-section that should be used for a specific bandpass of finite …
The multiwavelength picture of star formation in the very young open cluster NGC6383
G Rauw, M De Becker - arXiv preprint arXiv:0808.3887, 2008 - arxiv.org
We review the properties of the very young (2 Myr) open cluster NGC6383. The cluster is
dominated by the massive binary HD159176 (O7V+ O7V). The distance to NGC6383 is …
dominated by the massive binary HD159176 (O7V+ O7V). The distance to NGC6383 is …
3D reconstruction and visualization of astrophysical wind volumes using physical models
I Pachoulakis - ACM Transactions on Modeling and Computer …, 2008 - dl.acm.org
This article reports on the application of a framework used to model, simulate and visualize
the 3D structure of astrophysical wind volumes. The modeling methodology is similar to …
the 3D structure of astrophysical wind volumes. The modeling methodology is similar to …
Suzaku observations of the massive twin star HD159176
K Yamazaki, Y Tsuboi, M Tsujimoto… - The First Year of MAXI …, 2010 - adsabs.harvard.edu
HD159176 is a close binary system which is composed with O7V+ O7V type stars. The
system is in the young open cluster NGC6383 with a distance of about 1.5 kpc. With almost …
system is in the young open cluster NGC6383 with a distance of about 1.5 kpc. With almost …
[PDF][PDF] Resonant Ion Scattering and the Integrated Atomic Scattering Cross-section for Determining Ion densities in the Modeled Shock Fronts of EM Carinae and …
RJ Pfeiffer, T Wickramasinghe - owd.tcnj.edu
The current literature is rather vague regarding how to calculate the exact numerical value of
the resonant ion scattering cross section that should be used for a specific bandpass of finite …
the resonant ion scattering cross section that should be used for a specific bandpass of finite …
[PDF][PDF] Realistic Interactive Multimedia Generation using Physical Models–II. Visualizing the Stellar Wind Effective Envelopes
I Pachoulakis - researchgate.net
This is the second of two articles reporting on the generation of realistic multimedia content
and applications using physical models to increase the effectiveness and communication …
and applications using physical models to increase the effectiveness and communication …