Recent RXTE/ASM and ROTSEIIId observations of EXO 2030+375 (V2246 Cygni)

Creative Commons License

BAYKAL A., Kiziloglu U., Kiziloglu N., Beklen E., Oezbey M.

ASTRONOMY & ASTROPHYSICS, vol.479, no.2, pp.301-306, 2008 (SCI-Expanded, Scopus)

  • Publication Type: Article / Article
  • Volume: 479 Issue: 2
  • Publication Date: 2008
  • Doi Number: 10.1051/0004-6361:20078721
  • Journal Name: ASTRONOMY & ASTROPHYSICS
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Page Numbers: pp.301-306
  • Keywords: accretion, accretion disks, X-rays : stars, X-RAY PULSAR, TIME-SERIES ANALYSIS, OPTICAL COUNTERPART, EXO-2030+375, BINARY, OUTBURST, MULTIWAVELENGTH, MECHANISMS, DISCOVERY, ACCRETION
  • Open Archive Collection: AVESIS Open Access Collection
  • Middle East Technical University Affiliated: Yes

Abstract

Aims. Using the archival RXTE/ASM and SWIFT/BAT observations, the new orbital phases of type I outbursts of EXO 2030+375 are estimated. A possible correlation between the type II outburst and optical brightness variations is investigated.