pith. sign in

N.G. Beskrovnaya

Identifiers

  • name variant N.G. Beskrovnaya 0.60 · backfill

Papers (13)

  1. AR Scorpii is a new white dwarf in the ejector state astro-ph.HE · 2016 · author #1
  2. Features of the Matter Flows in the Peculiar Cataclysmic Variable AE Aquarii astro-ph.SR · 2016 · author #5
  3. A scenario of the formation of isolated X-ray pulsars with anomalously long period astro-ph.HE · 2014 · author #3
  4. On the origin of the peculiar cataclysmic variable AE Aquarii astro-ph.HE · 2014 · author #1
  5. Spin evolution of long-period X-ray pulsars astro-ph.HE · 2014 · author #3
  6. On the spin-down mechanism of the X-ray pulsar 4U 2206+54 astro-ph.HE · 2012 · author #2
  7. AE Aquarii represents a new subclass of Cataclysmic Variables astro-ph.HE · 2012 · author #2
  8. Signs of magnetic accretion in X-ray pulsars astro-ph.HE · 2012 · author #2
  9. On the energy release in solar flares astro-ph.SR · 2012 · author #3
  10. AE Aquarii: The first white dwarf in the family of spin-powered pulsars astro-ph · 2008 · author #2
  11. On the mass transfer in AE Aquarii astro-ph · 2004 · author #3
  12. On the circularly polarized optical emission from AE Aquarii astro-ph · 2002 · author #3
  13. On the accretion flow geometry in A0535+26 astro-ph · 2001 · author #3

Mentions

  • 1408.2397 #3 · backfill · confidence 0.70 N.G. Beskrovnaya
  • 1405.2182 #1 · backfill · confidence 0.70 N.G. Beskrovnaya
  • 1402.1029 #3 · backfill · confidence 0.70 N.G. Beskrovnaya
  • 1211.6314 #2 · backfill · confidence 0.70 N.G. Beskrovnaya
  • 1205.4330 #2 · backfill · confidence 0.70 N.G. Beskrovnaya
  • 1205.2846 #2 · backfill · confidence 0.70 N.G. Beskrovnaya
  • 1204.6594 #3 · backfill · confidence 0.70 N.G. Beskrovnaya
  • 0809.1169 #2 · backfill · confidence 0.70 N.G. Beskrovnaya

Frequent Coauthors