Difference between revisions of "XTE J1859+083"

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Pulse period clearly detected at 9.789s, with Matthias orbit (probably consistent with GBM results).
 
Pulse period clearly detected at 9.789s, with Matthias orbit (probably consistent with GBM results).
 
Spectrum best described by NPEX with black-body and FeKα line, but FDcut and cutoffpl also work.
 
Spectrum best described by NPEX with black-body and FeKα line, but FDcut and cutoffpl also work.
 +
 +
Actually NPEX and FDcut do not work as well as a cutoff with bb, judging from the number of parameters.

Latest revision as of 14:15, 1 February 2023


Monitoring data

Coordinates

Ra 284.75887 Dec 8.254142 NuSTAR observed coordinates
Ra 18h 59m 01.57s Dec +08d 14' 44.2" Coordinates in ATel #7067

Ephemeris

M. Kühnel from Fermi/GBM pulse periods:

P 37.9 ± 0.05 d
T0 MJD 57078.79 (+0.14, -0.06) periastron passage
a sin i 215.1 ± 0.4 lt-s
ε 0.1251 ± 0.017
ω -115.77 (+0.08, -0.16)

On the Fermi/GBM pulsar project website (on 2015-04-17)

P 38.176 d
T90 JD 2457063.048
a sin i 213.19 lt-s
ε 0.1309
ω ?

Pulse period around 9.8s [1].

Literature

Only one good paper: [1]. Postulated 60.65d orbit and found pulse period with 9.8s. RXTE spectra with typical pulsar spectrum, no CRSF. Recent 2015 data analysis by [2] with a focus on companion search.

Available data

NuSTAR observation on 2015, March 30/31, for 20ks. Pulse period clearly detected at 9.789s, with Matthias orbit (probably consistent with GBM results). Spectrum best described by NPEX with black-body and FeKα line, but FDcut and cutoffpl also work.

Actually NPEX and FDcut do not work as well as a cutoff with bb, judging from the number of parameters.

  1. 1.0 1.1 Corbet, R., in't Zand, J. J. M., Levine, A. M., Marshall, F. E., 2009, ApJ 695, 30 (NASA ADS)
  2. Salganik, A., Tsygankov, S. S., Djupvik, A. A., et al. “On the nature of the X-ray pulsar XTE J1859+083 and its broad-band properties”, 2022, MNRAS 509, 4 (NASA ADS)