2019ApJ...882...25P


Query : 2019ApJ...882...25P

2019ApJ...882...25P - Astrophys. J., 882, 25-25 (2019/September-1)

X-ray spectral evolution of PSR J2032+4127 during the 2017 periastron passage.

PAL P.S., TAM P.H.T., CUI Y., LI K.L., KONG A.K.H. and GUNGOR C.

Abstract (from CDS):

We report X-ray data analysis results obtained from Chandra, XMM-Newton, Nuclear Spectroscopic Telescope Array Mission (NuSTAR), and Swift observations of PSR J2032+4127 taken before, during, and after the periastron on 2017 November 13. We found the first clear evidence of a change in the X-ray spectral index over the passage period, thanks to a broad and sensitive spectral coverage by XMM-Newton and NuSTAR. We analyzed the joint XMM-Newton and NuSTAR observation epochs with power-law and broken power-law models. We have obtained changes in spectral parameters before and after the periastron passage for both models. The spectra get softened after the passage. The evolution of the spectral index and break energy before and after the periastron may indicate a change in the physical state of shock-accelerated electrons.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): pulsars: individual: PSR J2032+4127 - stars: individual: MT91 213 - stars: winds, outflows - X-rays: binaries

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 1FGL J1018.6-5856 HXB 10 18 55.5875706288 -58 56 45.975246900   13.638 12.683     O6V((f)) 156 0
2 CPD-63 2495 HXB 13 02 47.6544015048 -63 50 08.626970292 10.34 10.72 9.98 10.03   O9.5Ve 852 0
3 V* V479 Sct HXB 18 26 15.0561548880 -14 50 54.247274304 12.02 12.23 11.27 11.04   ON6V((f))z 613 2
4 [MT91] 213 Psr 20 32 13.1247390384 +41 27 24.346666440 13.12 13.08 11.266     B0Vp 334 0
5 Ass Cyg OB 2 As* 20 33.2 +41 19           ~ 1023 0

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