Quark Star Found?

4U 1746–37: An ultra-low-mass compact star candidate

Author:

Li

Abstract:

The Rossi X-ray Timing Explorer observed three photospheric radius expansion bursts in 4U 1746-37, all with low touchdown fluxes. We discuss the possibiity of a low-mass neutron star in 4U 1746-37 if the touchdown flux corresponds to its Eddington limit. 4U 1746-37 is a dipping binary system which has a high inclination angle. Two geometric effects, the reflection of the far side accretion disc and the obscuration of the near side accretion disc have also been included. We apply a Monte-Carlo simulation, with typical values of hydrogen mass fraction and color correction factor, to constrain the mass and radius of the neutron star in 4U 1746-37. We found that the mass of 4U 1746-37 is 0.41+0.70–0.30 M® at 99.7 % confidence which is an ultra-low-mass compact star candidate. It could be reproduced by a self-bound compact star, i.e., quark star or quark-cluster star, from an ccretion-induced collapse process.

First Quark Star Discovered?

An Ultra Low Mass and Small Radius Compact Object in 4U 1746-37?

Authors:

Li et al

Abstract:

Photospheric radius expansion (PRE) bursts have already been used to constrain the masses and radii of neutron stars. \textit{RXTE} observed three PRE bursts in \object{4U 1746-37}, all with low touchdown fluxes. We discuss here the possibility of low mass neutron star in \object{4U 1746-37} because the Eddington luminosity depends on stellar mass. With typical values of hydrogen mass fraction and color correction factor, a Monte-Carlo simulation was applied to constrain the mass and radius of neutron star in \object{4U 1746-37}. \object{4U 1746-37} has a high inclination angle. Two geometric effects, the reflection of the far side accretion disc and the obscuration of the near side accretion disc have also been included in the mass and radius constraints of \object{4U 1746-37}. If the reflection of the far side accretion disc is accounted, a low mass compact object (mass of 0.61±0.14 M⊙ and radius of 10.46±0.61 km at 68% confidence) exists in \object{4U 1746-37}. If the another effect operated, \object{4U 1746-37} may contain an ultra low mass and small radius object (M=0.27±0.08 M⊙, R=7.47±0.60 km at 68% confidence), which could be reproduced by a self-bound compact star, i.e., quark star or quark cluster star.