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Astronomy an astrophysica
Phase-free spectroscopic analysis of the darkening black hole X-ruggeder M33 X-7: System properties, accretion and evolution
Helge Todt
M33 x-7 there the Eneste Formørkelse Af sort hul med høj masse røntgenbinær.Systemet Raporteres at Indholte and Meget Massiv o Supergiant -Donor OG et Massivt sort hul I and short bane. The high x-ray luminosity and location-Poor Galaxy M33 makes it a unique laboratory for studying the wind of metal -poor donor stars with black hole mates and it helps us to understand the potential precursors of Black Hole Fusions.Ved Hjælp Af PhasePløst samtidige HST-Oog XMM-Newton observationer We are followed the interaction between the star wind with the black hole.We have observed a strong Hatchett-MCray effect in the M33 X-7 for the entire spectrum of wind speeds.Onze uitgebreide spectroscopisch onderzoek van de donorster (X-ray+UV +Optical) Yields New Stellar and Wind Parameters for the System That Differ Significantly from Previous Estimates.isar The masses of the components are significantly reduced to ≈38 M⊙ for the O-Star Donor and -11.4 M⊙ For the Black Hole.o Gian ...
Measurement of stellar wind parameters in IGR J17544-2619 and VELA X-1 limits the accretion physics in super giants Fast X-ray outbursts and classic super giants X-rugging stars
2016 •
J. J. Rodes
Classic Supergiant X -Ray Binaries (SGXBS) and Supergiant Fast X -Rays (SFXTS) are two that have been suggested, some of them specific to the specific stars of the donor stars. Kun Dedicated empirical analysis of the donors' stellar wind may provide the required information to perform a suitableTesting these theories. However, such analyzes are scarce. To close this gap we perform a comparative analysis of the optical Companion in Two Important Systems: IGR J17544-2619 (SFXT) and VELA X-1 (SGXB) .we Analysis The Spectraof Each Star in Detail and Derive Their Stellar and Wind Properties.we Compare The Wind Parameters, Giving Us An Excellent Chance van het herkennen van belangrijke verschillen tussen donorwinden in SFXT's en SGXB's ...
Astronomy an astrophysica
X-ray emissions of hydrodynamic simulations in non-LTE wind models
2009 •
Jiří Kubát
Space science reviews
Against a united image of inhom*ogenic star winds in insulated Supergiant stars and Supergant High Pulp X series
2017 •
Peter Blay
Astronomy an astrophysica
XMM-Newton spectroscopy of the growing Magnetar candidate 4h0114+65
Guillermo Bernabéu
Astronomy an astrophysica
Magnetorotation -instability in limiting discs of critically rotating stars and the outer structure of BE and Bestwile
2014 •
Peter Kurfürst
Astronomy an astrophysica
Cosmic herionization of primordial cosmic rays
2014 •
Matias
Journal of Dental Research
Nuclear F-Actin Cytology in oral epithelial dysplasia and oral plate cell carcinoma
2020 •
N. Vigneswaran
The oral cavity cancer has a low 5-year-old overcoly rate rate, but the results are improved when the disease is detected early. Cytology is a less invasive method for Bij Assessing Oral Potential Histile Haadilt Haadilt Haadilt Haadilt Haadilt Haadilt Haadilt Haadilt Haadilt HaadilthaadiLt haadiLt haadiLt haadiLt haadiLt HandtoLtaDiLt HaVeDiLt HaVeDiLt HaVeDiLt Handel Tildstand Skalbiopsi.Il purpose up determining the use of cytological signatures, including nuclear f-actin cell phenotypes, for classification of the full spectrum of oral epithelial dysplasia and oral record cell carcinoma et Verkregen Borstelcytology Specimens a Gematchte Scalpelbiopsies van 486 Proefersen.Histopathology Beoordelings van Scalpel Biopsys -Geclassificerde Laesies in 6 Categoryën.
Research in astronomy and astrophysics
About the possibility of disk-fed formation in Supergant High Massa Radio Cinars
2019 •
Dr.Ali Taani
Research into astronomy and astrophysics
About the possibility of disk-fed formation in SuperGiant-Röntgevlubbelstars with high mass.pdf
2019 •
Dr.Ali Taani,,Mohammed K.Mardini
We have considered the existence of neutron star -magnet field given by the cyclotron lines.We collected the data from 9 sources to radio -ray with high mass with supergiant accompanies as a case of testing our model to demonstrate their distribution and development.The wind speed, spin period and magnetic field strength are studied at different mass losses..Vores Model laat zien dat de meeste bronnen (6 AF9 -systemen) kunnen worden gevoed door de wind met relatief lage snelheid, en dit resultaat is in lijn met eerdere voorspellingen.Track van Verschillende soorten binaire stock, waardoor one Duidelijk Dichotomy Right Wordt Getoond In Windgeboren X -Ray -Binaire System.
