Reanalysis of high-resolution XMM-Newton data of V2491 Cygni using models of collisionally ionized hot absorbers

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Balman S., Gamsizkan C.

ASTRONOMY & ASTROPHYSICS, cilt.598, 2017 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 598
  • Basım Tarihi: 2017
  • Doi Numarası: 10.1051/0004-6361/201629360
  • Dergi Adı: ASTRONOMY & ASTROPHYSICS
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Anahtar Kelimeler: X-rays: stars, stars: individual: V2491 Cyg, binaries: general, novae, cataclysmic variables, stars: abundances, stars: winds, outflows, X-RAY-EMISSION, PHOTON IMAGING CAMERA, NOVA V382 VELORUM, RECURRENT NOVA, CLASSICAL NOVA, GRATING SPECTROMETER, PROGENITOR SYSTEM, 2006 OUTBURST, WHITE-DWARFS, V1974 CYGNI
  • Orta Doğu Teknik Üniversitesi Adresli: Evet

Özet

Aims. We model spectral absorption features in data of the high-resolution XMM-Newton Reflection Grating Spectrometer.