Contains fulltext : 33048.pdf ( ) (Open Access) Contains fulltext : 33048.pdf (publisher's version ) (Open Access)We present the results of XMM-Newton observations of four AM CVn systems - AM CVn, CR Boo, HP Lib and GP Com. Their light curves show very different characteristics. The X-ray light curves show no coherent pulsations, suggesting the accreting white dwarfs have relatively low magnetic field strengths. Their spectra were best modelled using a multi-temperature emission model and a strong UV component. We find tha
We present a comparative study of X-ray emission from a sample of active M dwarfs with spectral type...
To appear in the Proceedings of "The Golden Age of Cataclysmic Variables (Palermo 2011)", in Mem. So...
The unusual variable star AM CVn has puzzled astronomers for over 40 years. This object, both a phot...
We present the results of XMM-Newton observations of four AM CVn systems - AM CVn, CR Boo, HP Lib an...
We present the results of XMM-Newton observations of four AM CVn systems – AM CVn, CR Boo, HP Lib an...
Contains fulltext : 34840.pdf ( ) (Open Access) ...
We present the results of XMM-Newton observations of two AM CVn systems - V396 Hya and SDSS J1240-01...
We present the results of XMM-Newton observations of two AM CVn systems - V396 Hya and SDSS J1240-01...
We present the results of XMM-Newton observations of two AM CVn systems - V396 Hya and SDSS J1240-01...
Contains fulltext : 36392.pdf ( ) (Open Access)We present the results of some rece...
The AM CVn systems are a class of He-rich, post-period minimum, semi-detached, ultra-compact binarie...
We present the results of some recent research on AM CVn systems. We present: X-ray/UV observations ...
AM CVn binaries are hydrogen deficient compact binaries with an orbital period in the 5–65 min range...
We calculate the heating and cooling of the accreting white dwarf (WD) in the ultracompact AM Canum ...
We present a comparative study of X-ray emission from a sample of active M dwarfs with spectral type...
To appear in the Proceedings of "The Golden Age of Cataclysmic Variables (Palermo 2011)", in Mem. So...
The unusual variable star AM CVn has puzzled astronomers for over 40 years. This object, both a phot...
We present the results of XMM-Newton observations of four AM CVn systems - AM CVn, CR Boo, HP Lib an...
We present the results of XMM-Newton observations of four AM CVn systems – AM CVn, CR Boo, HP Lib an...
Contains fulltext : 34840.pdf ( ) (Open Access) ...
We present the results of XMM-Newton observations of two AM CVn systems - V396 Hya and SDSS J1240-01...
We present the results of XMM-Newton observations of two AM CVn systems - V396 Hya and SDSS J1240-01...
We present the results of XMM-Newton observations of two AM CVn systems - V396 Hya and SDSS J1240-01...
Contains fulltext : 36392.pdf ( ) (Open Access)We present the results of some rece...
The AM CVn systems are a class of He-rich, post-period minimum, semi-detached, ultra-compact binarie...
We present the results of some recent research on AM CVn systems. We present: X-ray/UV observations ...
AM CVn binaries are hydrogen deficient compact binaries with an orbital period in the 5–65 min range...
We calculate the heating and cooling of the accreting white dwarf (WD) in the ultracompact AM Canum ...
We present a comparative study of X-ray emission from a sample of active M dwarfs with spectral type...
To appear in the Proceedings of "The Golden Age of Cataclysmic Variables (Palermo 2011)", in Mem. So...
The unusual variable star AM CVn has puzzled astronomers for over 40 years. This object, both a phot...