Institutional Repository

Browsing Work in progress by Subject "Magellanic Clouds; X-rays: binaries; X-rays: galaxies; X-rays: general Active galactic nuclei; Be Stars; Hydrogen column density; Magellanic Clouds; Optical spectroscopy; Small magellanic clouds; Systematic analysis; X ray binaries; X-ray energies; X-ray pulsars; X-ray sources; X-rays: binaries; X-rays: Galaxies; X-rays: general; XMM-Newton; XMM-Newton observations; Galaxies; Population statistics; Stars; X ray optics; X rays"

Browsing Work in progress by Subject "Magellanic Clouds; X-rays: binaries; X-rays: galaxies; X-rays: general Active galactic nuclei; Be Stars; Hydrogen column density; Magellanic Clouds; Optical spectroscopy; Small magellanic clouds; Systematic analysis; X ray binaries; X-ray energies; X-ray pulsars; X-ray sources; X-rays: binaries; X-rays: Galaxies; X-rays: general; XMM-Newton; XMM-Newton observations; Galaxies; Population statistics; Stars; X ray optics; X rays"

Sort by: Order: Results:

  • Novara G.; La Palombara N.; Mereghetti S.; Haberl F.; Coe M.; Filipovic M.; Udalski A.; Paizis A.; Pietsch W.; Sturm R.; Gilfanov M.; Tiengo A.; Payne J.; Smits D.; De Horta A. (2011)
    Many of the high mass X-ray binaries (HMXRBs) discovered in recent years in our Galaxy are characterized by a high absorption, most likely intrinsic to the system, that can impede their detection at the softest X-ray ...

Search UnisaIR


Browse

My Account