Accretion in strong field gravity with eXTP


Creative Commons License

De Rosa A., Uttley P., Gou L., Liu Y., Bambi C., Barret D., ...Daha Fazla

SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, cilt.62, sa.2, 2019 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Derleme
  • Cilt numarası: 62 Sayı: 2
  • Basım Tarihi: 2019
  • Doi Numarası: 10.1007/s11433-018-9297-0
  • Dergi Adı: SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Anahtar Kelimeler: X-ray, black holes physics, accretion, QUASI-PERIODIC OSCILLATIONS, BLACK-HOLE SPIN, X-RAY BINARIES, LENS-THIRRING PRECESSION, ACTIVE GALACTIC NUCLEI, ULTRA-FAST OUTFLOWS, XMM-NEWTON, IRON K, ELECTROMAGNETIC EMISSION, SPECTRAL FEATURES
  • Orta Doğu Teknik Üniversitesi Adresli: Evet

Özet

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced "spectral-timing-polarimetry" techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful out flows which are driven by the accretion process.