http://arxiv.org/abs/2209.00911
The millisecond pulsar MAXI J1816–195 was recently discovered by MAXI in 2022 May. We have studied different properties of the pulsar using data from NuSTAR and NICER observations. The position of the source is measured by NuSTAR as RA = $18^h 16^m 52^s.40$, Dec = $-19^o37^{‘} 58^{”}.35$. The unstable burning of accreted material on the surface of neutron stars induces thermonuclear (Type-I) bursts. Several thermonuclear bursts have been detected from the source during the outburst. We study the evolution of burst profile with flux and energy using NuSTAR and NICER observations. During the NuSTAR observation, a total of four bursts were detected from the source. The duration of each burst was around $\sim$ 30 s and the ratio of peak to persistent count rate is $\sim$ 26 as seen from the NuSTAR data. The thermonuclear bursts are modeled to determine the burst timing parameters using a sharp linear rise and exponential decay function. The burst profiles show a relatively long tail in lower energies. The hardness ratio during the thermonuclear bursts shows significant variation as observed by NuSTAR. We successfully model the broadband burst-resolved spectra with a combination of an absorbed blackbody along with a non-thermal component to account for the persistent emission. The burst-resolved spectral parameters show significant evolution during the burst. During the peak of the burst, the Eddington luminosity is found to be $\sim 3.7 \times 10^{38}$ erg s$^{-1}$. The burst-resolved spectral parameters provide a source distance of $8.5\pm1.2$ kpc for isotropic burst emission.
M. Mandal, S. Pal, J. Chauhan, et. al.
Mon, 5 Sep 22
53/53
Comments: 13 pages, 9 figures, 4 tables, comments are welcome
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