Revised physical elements of the astrophysically important O9. 5+ O9. 5V eclipsing binary system Y Cygni
P Harmanec, DE Holmgren, M Wolf, H Božić… - Astronomy & …, 2014 - aanda.org
Context. Rapid advancements in light-curve and radial-velocity curve modelling, as well as
improvements in the accuracy of observations, allow more stringent tests of the theory of …
improvements in the accuracy of observations, allow more stringent tests of the theory of …
[HTML][HTML] New apsidal-motion parameters for Y Cygni
D Holmgren, G Hill, CD Scarfe - … , vol. 115, p. 188-192 (1995), 1995 - adsabs.harvard.edu
New apsidal-motion parameters for Y Cygni ADS Classic is now deprecated. It will be completely
retired in October 2019. This page will automatically redirect to the new ADS interface at that …
retired in October 2019. This page will automatically redirect to the new ADS interface at that …
Polarimetric measures of selected variable stars
NM Elias, RH Koch, RJ Pfeiffer - Astronomy & Astrophysics, 2008 - aanda.org
Aims. The purpose of this paper is to summarize and interpret unpublished optical
polarimetry for numerous program stars that were observed over the past decades at the …
polarimetry for numerous program stars that were observed over the past decades at the …
HD 159176: photospheric and wind-dominated light-curve analyses coupled to wind modelling
I Pachoulakis - Monthly Notices of the Royal Astronomical …, 1996 - academic.oup.com
HD 159176 is a hot, massive, non-eclipsing binary with a small-amplitude ellipsoidal
variability. The existing velocity solution determines the ratio of the stellar masses. In the …
variability. The existing velocity solution determines the ratio of the stellar masses. In 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 winds of hot close binaries. Paper 3: HD 159176
RJ Pfeiffer, I Pachoulakis, RH Koch… - The Observatory, vol …, 1997 - adsabs.harvard.edu
A binary-star wind-interaction (BWI) computer code has been developed to account for the
eclipsing and radiative-transfer interactions among the winds and photospheres of a close …
eclipsing and radiative-transfer interactions among the winds and photospheres of a close …
[HTML][HTML] The winds of hot close binaries. Paper 2: CW Cephei (HD 218066)
I Pachoulakis, RJ Pfeiffer, RH Kock… - … , v. 116, p. 89-97 (1996 …, 1996 - adsabs.harvard.edu
The winds of hot close binaries. Paper 2: CW Cephei (HD 218066) ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
[HTML][HTML] The winds of hot, close binaries. Paper 4: EM Carinae (HD 97484)
RJ Pfeiffer, DJ Stickland - The Observatory, Vol. 124, p. 117 …, 2004 - adsabs.harvard.edu
The winds of hot, close binaries. Paper 4: EM Carinae (HD 97484) ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
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 …
[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 …