The Megasecond Chandra X-Ray Visionary Project Observation of NGC 3115 (II): properties of point sources
arXiv:1506.05448 · doi:10.1088/0004-637X/808/1/19
Abstract
We have carried out an in-depth study of low-mass X-ray binaries (LMXBs) detected in the nearby lenticular galaxy NGC 3115, using the Megasecond Chandra X-Ray Visionary Project observation (total exposure time 1.1 Ms). In total we found 136 candidate LMXBs in the field and 49 in globular clusters (GCs) above 2σ detection, with 0.3--8 keV luminosity L_X ~10^36-10^39 erg/s. Other than 13 transient candidates, the sources overall have less long-term variability at higher luminosity, at least at L_X > 2x10^37 erg/s. In order to identify the nature and spectral state of our sources, we compared their collective spectral properties based on single-component models (a simple power law or a multicolor disk) with the spectral evolution seen in representative Galactic LMXBs. We found that in the L_X versus photon index Γ_PL and L_X versus disk temperature kT_MCD plots, most of our sources fall on a narrow track in which the spectral shape hardens with increasing luminosity below L_X~7x10^37 erg/s but is relatively constant (Γ_PL~1.5 or kT_MCD~1.5 keV) above this luminosity, similar to the spectral evolution of Galactic neutron star (NS) LMXBs in the soft state in the Chandra bandpass. Therefore we identified the track as the NS LMXB soft-state track and suggested sources with L_X<7x10^37 erg/s as atolls in the soft state and those with L_X>7x10^37 erg/s as Z sources. Ten other sources (five are transients) displayed significantly softer spectra and are probably black hole X-ray binaries in the thermal state. One of them (persistent) is in a metal-poor GC.
26 pages, 9 figures, four online tables, accepted for publication in ApJ
References in corpus (18)
- X-ray Properties of Black-Hole Binaries
- Modelling the behaviour of accretion flows in X-ray binaries
- Thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer
- A Long, Hard Look at the Low-Hard State in Accreting Black Holes
- Stellar populations of early-type galaxies in different environments II. Ages and metallicities
- Testing Accretion Disk Theory in Black Hole X-ray Binaries
- Evaluating Spectral Models and the X-ray States of Neutron-Star X-ray Transients
- A new method for determining the sensitivity of X-ray imaging observations and the X-ray number counts
- A Grid of Relativistic, non-LTE Accretion Disk Models for Spectral Fitting of Black Hole Binaries
- Chandra Multiwavelength Project X-ray Point Source Catalog
- X-ray irradiation in XTE J1817-330 and the inner radius of the truncated disc in the hard state
- Intermittent pulsations in an accretion-powered millisecond pulsar
- Models for Low-Mass X-Ray Binaries in the Elliptical Galaxies NGC3379 and NGC4278: Comparison with Observations
- Common Patterns in the Evolution between the Luminous Neutron Star Low-Mass X-ray Binary Subclasses
- The SLUGGS Survey: HST/ACS Mosaic Imaging of the NGC 3115 Globular Cluster System
- The Remarkable Stability of Probable Black Hole Low-Mass X-ray Binaries in Nearby Galaxies
- 50 M31 black hole candidates identified by Chandra and XMM-Newton
- The Megasecond Chandra X-Ray Visionary Project Observation of NGC 3115 (III): luminosity functions of LMXBs and dependence on stellar environments
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