A multi-model approach to X-ray pulsars Connecting spectral and timing models to pin down the intrinsic emission characteristics of magnetized, accreting neutron stars

  1. Schoenherr, G.
  2. Schwarm, F.
  3. Falkner, S.
  4. Becker, P.
  5. Wilms, J.
  6. Dauser, T.
  7. Wolff, M. T.
  8. Wolfram, K.
  9. West, B.
  10. Pottschmidt, K.
  11. Kretschmar, P.
  12. Ferrigno, C.
  13. Klochkov, D.
  14. Nishimura, O.
  15. Kreykenbohm, I.
  16. Caballero, I.
  17. Staubert, R.
Liburu bilduma:
PHYSICS AT THE MAGNETOSPHERIC BOUNDARY
  1. Bozzo, E (coord.)
  2. Kretschmar, P (coord.)
  3. Audard, M (coord.)
  4. Falanga, M (coord.)
  5. Ferrigno, C (coord.)

ISSN: 2100-014X

ISBN: 978-2-7598-1143-4

Argitalpen urtea: 2014

Alea: 64

Biltzarra: Conference on Physics at the Magnetospheric Boundary

Mota: Biltzar ekarpena

DOI: 10.1051/EPJCONF/20146402003 GOOGLE SCHOLAR