A STRONGLY HEATED NEUTRON STAR IN THE TRANSIENT Z SOURCE MAXI J0556-332
We present Chandra, XMM-Newton, and Swift observations of the quiescent neutron star in the transient low-mass X-ray binary MAXI J0556-332. Observations of the source made during outburst (with the Rossi X-ray Timing Explorer) reveal tracks in its X-ray color-color and hardness-intensity diagrams th...
Main Authors: | Homan, Jeroen, Fridriksson, Joel K., Wijnands, Rudy, Cackett, E. M., Degenaar, N., Linares, Manuel Alegret, Lin, Dacheng, Remillard, Ronald A |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2015
|
Online Access: | http://hdl.handle.net/1721.1/94549 |
Similar Items
-
The nature of the X-ray transient MAXI J0556-332
by: Cornelisse, R, et al.
Published: (2012) -
TYPE I X-RAY BURSTS FROM THE NEUTRON-STAR TRANSIENT XTE J1701–462
by: Lin, Dacheng, et al.
Published: (2015) -
DISCOVERY OF THE NEAR-INFRARED COUNTERPART TO THE LUMINOUS NEUTRON-STAR LOW-MASS X-RAY BINARY GX 3+1
by: van den Berg, Maureen, et al.
Published: (2015) -
COMMON PATTERNS IN THE EVOLUTION BETWEEN THE LUMINOUS NEUTRON STAR LOW-MASS X-RAY BINARY SUBCLASSES
by: Homan, Jeroen, et al.
Published: (2015) -
ON THE GEOMETRIC NATURE OF LOW-FREQUENCY QUASI-PERIODIC OSCILLATIONS IN NEUTRON-STAR LOW-MASS X-RAY BINARIES
by: Homan, Jeroen, et al.
Published: (2015)