Future Prospects for Ultra-High Resolution Imaging of Binary Systems at UV and X-ray Wavelengths

@article{Karovska2006FuturePF,
  title={Future Prospects for Ultra-High Resolution Imaging of Binary Systems at UV and X-ray Wavelengths},
  author={Margarita Karovska},
  journal={Astrophysics and Space Science},
  year={2006},
  volume={304},
  pages={379-382}
}
  • M. Karovska
  • Published 19 September 2006
  • Physics
  • Astrophysics and Space Science
UV and X-ray space-based interferometry will open unprecedented possibilities for spectral and spatial studies of a wide range of currently unresolvable interacting systems. Ultra-high angular resolution direct imaging of individual} components and transport processes in interacting binary systems is essential for detailed studies and modeling of accretion and activity. Understanding the mass loss characteristics of both components, and the dynamics of the system as a function of time, will… 
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References

SHOWING 1-5 OF 5 REFERENCES
First Hubble Space Telescope Observations of Mira AB Wind-accreting Binary System
The Mira AB system belongs to a class of detached binaries in which a compact object accretes mass from the wind of a cool giant or supergiant. This system provides a unique laboratory for detailed
A large X-ray outburst in Mira A
We report the Chandra ACIS-S detection of a bright soft X-ray transient in the Mira AB interacting symbiotic-like binary. We have resolved the system for the first time in X-rays. Using Chandra and
The Large-Scale Ionized Outflow of CH Cygni*
Hubble Space Telescope (HST) and ground-based [O II] and [N II] images obtained in the period 1996-1999 reveal a complex, ionized optical nebula around the symbiotic binary CH Cyg extending out to
Type-Ia supernovae in dense circumstellar gas
We propose a model for the bolometric light curve of a type-Ia supernova (SN Ia) that explodes in a dense circumstellar (CS) envelope. Our modeling of the light curves for SN 2002ic and SN 1997cy