A variable near-infrared counterpart to the neutron-star low-mass X-ray binary 4U 1705-440
arXiv:0811.1494 · doi:10.1088/0004-637X/692/1/73
Abstract
We report the discovery of a near-infrared (nIR) counterpart to the persistent neutron-star low-mass X-ray binary 4U 1705-440, at a location consistent with its recently determined Chandra X-ray position. The nIR source is highly variable, with K_s-band magnitudes varying between 15.2 and 17.3 and additional J- and H-band observations revealing color variations. A comparison with contemporaneous X-ray monitoring observations shows that the nIR brightness correlates well with X-ray flux and X-ray spectral state. We also find possible indications for a change in the slope of the nIR/X-ray flux relation between different X-ray states. We discuss and test various proposed mechanisms for the nIR emission from neutron-star low-mass X-ray binaries and conclude that the nIR emission in 4U 1705-440 is most likely dominated by X-ray heating of the outer accretion disk and the secondary star.
Accepted for publication in ApJ
References in corpus (6)
- Thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer
- Global optical/infrared - X-ray correlations in X-ray binaries: quantifying disc and jet contributions
- Evaluating Spectral Models and the X-ray States of Neutron-Star X-ray Transients
- Evidence for a jet contribution to the optical/infrared light of neutron star X-ray binaries
- Spitzer Reveals Infrared Optically-Thin Synchrotron Emission from the Compact Jet of the Neutron Star X-Ray Binary 4U 0614+091
- BeppoSAX observation of 4U 1705-44: detection of hard X-ray emission in the soft state
Cited by in corpus (12)
- XTE J1701-462 and its Implications for the Nature of Subclasses in Low-Magnetic-Field Neutron Star Low-Mass X-Ray Binaries
- A self-consistent approach to the hard and soft states of 4U 1705-44
- Suzaku and BeppoSAX X-ray Spectra of the Persistently Accreting Neutron-Star Binary 4U 1705-44
- The Spectral and Temporal Properties of Transient Sources in Early-Type Galaxies
- Discovery of the near-infrared counterpart to the luminous neutron-star low-mass X-ray binary GX 3+1
- The Chaotic Long-term X-ray Variability of 4U 1705--44
- Large amplitude variability from the persistent ultracompact X-ray binary in NGC 1851
- X-ray variability with spectral state transitions in NS-LMXBs observed with MAXI/GSC and Swift/BAT
- The Megasecond Chandra X-Ray Visionary Project Observation of NGC 3115 (II): properties of point sources
- A Transient Sub-Eddington Black Hole X-ray Binary Candidate in the Dust Lanes of Centaurus A
- The near-infrared counterpart of 4U 1636-53
- On the origin of the near-infrared emission from the neutron-star low-mass X-ray binary GX 9+1