Comprehensive analysis of the transient X-ray pulsar MAXI J1409−619

ABSTRACT We probe the properties of the transient X-ray pulsar MAXI J1409−619 through RXTE and Swift follow-up observations of the outburst in 2010. We are able to phase-connect the pulse arrival times for the 25 d episode during the outburst. We suggest that either an orbital model (with Porb ≃ 14....

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2020-08, Vol.496 (2), p.1768-1783
Hauptverfasser: Dönmez, Ç K, Serim, M M, İnam, S Ç, Şahiner, Ş, Serim, D, Baykal, A
Format: Artikel
Sprache:eng
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