J/A+A/706/A175      Pulsar Vela X-1 Pulse-to-Pulse Approach          (Du+, 2026)

Long-Term evolution of cyclotron resonant scattering features in the accreting pulsar Vela X-1: A pulse-to-pulse approach. Du Y.-J., Wang P.-J., Ducci L., Ji L., Kong L.-D., Bu Q.-C., Mehrotra C., Santangelo A. <Astron. Astrophys. 706, A175 (2026)> =2026A&A...706A.175D 2026A&A...706A.175D (SIMBAD/NED BibCode)
ADC_Keywords: Pulsars ; Accretion ; Gamma rays Keywords: accretion, accretion disks - pulsars: general Abstract: We investigated the long-term evolution of the cyclotron line energy, as well as the relationship between cyclotron line energy and luminosity in the high-mass X-ray binary Vela X-1, based on archival Swift/BAT monitoring from 2005 to 2024 and pulse-to-pulse analysis of nine NuSTAR observations from 2012 to 2024. Our results provide the first confirmation that the long-term decay of the harmonic line energy (Ecyc,H) in Vela X-1 has ended. We further report the first detection of a transient increase in Ecyc,H between 2020 and 2023, which suggests a sudden and significant change in the magnetic field configuration or accretion geometry. In addition, Ecyc,H shows slightly lower values at low luminosities and tends to flatten at higher luminosities, in the range of (0.13-1.21)x1037erg/s. The fundamental line energy (Ecyc,F) exhibits no significant variation with time or luminosity, remaining stable at approximately 25keV. Description: This catalogue contains the spectral parameters reported in Tables A.1-A.7 of the paper. The tables provide long-term Swift/BAT spectral results, NuSTAR time-averaged spectral result, and pulse-to-pulse spectral results for five NuSTAR observations. All uncertainties represent the 68% confidence level. Objects: ------------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------------ 09 02 06.86 -40 33 16.8 Vela X-1 = CD-40 4838 ------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 91 75 Best-fitting parameters of Vela X-1 from Swift/BAT monitoring tablea2.dat 252 23 NuSTAR phase-averaged spectra (eight observations) tablea3.dat 141 23 Pulse-to-pulse spectra for ObsID 10002007001 tablea4.dat 141 23 Pulse-to-pulse spectra for ObsID 30002007003 tablea5.dat 141 23 Pulse-to-pulse spectra for ObsID 30501003002 tablea6.dat 141 23 Pulse-to-pulse spectra for ObsID 90402339002 tablea7.dat 113 23 Pulse-to-pulse spectra for ObsID 91002349002 -------------------------------------------------------------------------------- See also: J/A+A/377/925 : Radial velocity curves of Vela X-1 (Barziv+, 2001) J/A+A/395/129 : Cyclotron lines in Vela X-1 (Kreykenbohm+, 2002) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Time Modified Julian Date interval of each spectrum (MJD) 13- 16 F4.2 keV kTComp Comptonizing plasma temperature 18- 21 F4.2 keV e_kTComp Lower error on kTComp 23- 26 F4.2 keV E_kTComp Upper error on kTComp 28- 32 F5.2 --- tauComp Compton optical depth 34- 37 F4.2 --- e_tauComp Lower error on tauComp 39- 42 F4.2 --- E_tauComp Upper error on tauComp 44- 48 F5.2 --- EcyclH Centroid energy of the harmonic CRSF 50- 53 F4.2 --- e_EcyclH Lower error on EcyclH 55- 58 F4.2 --- E_EcyclH Upper error on EcyclH 60- 64 F5.2 keV sigmaH Width of the harmonic CRSF 66- 69 F4.2 keV e_sigmaH Lower error on sigmaH 71- 74 F4.2 keV E_sigmaH Upper error on sigmaH 76- 80 F5.2 keV DepthH Line depth of the harmonic CRSF 82- 86 F5.2 keV e_DepthH Lower error on DepthH 88- 91 F4.2 keV E_DepthH Upper error on DepthH -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 28 A28 -- Param Name of parameter as defined in the paper (G1) 30- 56 A27 --- ObsID1 Value for ObsID = 10002007001 58- 84 A27 --- ObsID2 Value for ObsID = 30002007002 86-112 A27 --- ObsID3 Value for ObsID = 30002007003 114-140 A27 --- ObsID4 Value for ObsID = 90402339002 142-168 A27 --- ObsID5 Value for ObsID = 30501003002 170-196 A27 --- ObsID6 Value for ObsID = 90602328002 198-224 A27 --- ObsID7 Value for ObsID = 90602328004 226-252 A27 --- ObsID8 Value for ObsID = 90602328006 -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 29 A29 --- Param Spectral parameter names (G1) 31- 57 A27 --- 6769-9636 Best-fit values for 6769-9636 [ct/pulse] amplitude range 59- 85 A27 --- 9636-13580 Best-fit values for 9636-13580 [ct/pulse] amplitude range 87-113 A27 --- 1358-16240 Best-fit values for 1358-16240 [ct/pulste] amplitude range 115-141 A27 --- 1624-27083 Best-fit values for 1624-27083 [ct/pulste] amplitude range -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 29 A29 --- Param Spectral parameter names (G1) 31- 57 A27 --- 304-2108 Best-fit values for 304-2108 [ct/pulse] amplitude range 59- 85 A27 --- 2108-2557 Best-fit values for 2108-2557 [ct/pulse] amplitude range 87-113 A27 --- 2557-3422 Best-fit values for 2557-3422 [ct/pulste] amplitude range 115-141 A27 --- 3422-6340 Best-fit values for 3422-6340 [ct/pulste] amplitude range -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 29 A29 --- Param Spectral parameter names (G1) 31- 57 A27 --- 3113-5287 Best-fit values for 3113-5287 [ct/pulse] amplitude range 59- 85 A27 --- 5287-6693 Best-fit values for 5287-6693 [ct/pulse] amplitude range 87-113 A27 --- 6693-8728 Best-fit values for 6693-8728 [ct/pulste] amplitude range 115-141 A27 --- 8728-18521 Best-fit values for 8728-18521 [ct/pulste] amplitude range -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 29 A29 --- Param Spectral parameter names (G1) 31- 57 A27 --- 372-2639 Best-fit values for 372-2639 [ct/pulse] amplitude range 59- 85 A27 --- 2639-3581 Best-fit values for 2639-3581 [ct/pulse] amplitude range 87-113 A27 --- 3581-4382 Best-fit values for 3581-4382 [ct/pulste] amplitude range 115-141 A27 --- 4382-14043 Best-fit values for 4382-14043 [ct/pulste] amplitude range -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 29 A29 --- Param Spectral parameter names (G1) 31- 57 A27 --- 246-3098 Best-fit values for 246-3098 [ct/pulse] amplitude range 59- 85 A27 --- 3098-5884 Best-fit values for 3098-5884 [ct/pulse] amplitude range 87-113 A27 --- 5884-12359 Best-fit values for 5884-1235 [ct/pulste] amplitude range -------------------------------------------------------------------------------- Global notes: Note (G1): Parameters: C_FPMA : Cross-calibration constant of FPMA (fixed to 1) C_FPMB : Cross-calibration constant between FPMB and FPMA NH1 : Galactic absorption column density (fixed) NH2 : Partial-covering absorption column density CF : Covering fraction of the partial absorber E_10keV : Centroid energy of the 10keV feature (keV) σ_10keV : Width (Gaussian σ) of the 10keV feature (keV) Norm_10keV : Normalization of the 10keV feature E_Kalpha : Energy of the Fe Kα emission line (keV) sigma_Kalpha : Width (Gaussian sigma) of the Fe Kα line(keV) Norm_Kalpha : Normalization of the Fe Kα line EcycF : Fundamental cyclotron line energy(keV) sigmacycF : Width of the fundamental CRSF (fixed to 0.5 x sigmacycH) (keV) dcycF : Depth of the fundamental CRSF EcycH : Centroid energy of the harmonic CRSF(keV) sigmacycH : Width of the harmonic CRSF(keV) dcycH : Depth of the harmonic CRSF E_cut : Cutoff energy of the fdcut continuum(keV) E_fold : Folding energy of the fdcut continuum(keV) Gamma : Photon index of the power-law continuum Norm_Gamma : Power-law normalization Flux_3-79 keV_ : Unabsorbed flux in units of 10-9erg/cm2/s χ2/d.o.f. : Fit statistic and degrees of freedom All reported errors are at the 68% confidence level and based on the MCMC chain values. Normalization of the power law in units of photon/cm2/s/keV at 1keV. Unabsorbed flux (in units of 10-9erg/cm2/s) calculated for the entire model, obtained using the cflux command from xspec. Uncertainties are given for a 68% confidence level -------------------------------------------------------------------------------- Acknowledgements: Yujia Du, du(at)astro.uni-tuebingen.de, Institut fuer Astronomie und Astrophysik, Universitaet Tuebingen
(End) Yujia Du [Tuebingen Univ.], Patricia Vannier [CDS] 08-Dec-2025
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line