ON THE ORIGIN OF THE NEAR-INFRARED EMISSION FROM THE NEUTRON-STAR LOW-MASS X-RAY BINARY GX 9+1
We have determined an improved position for the luminous persistent neutron-star low-mass X-ray binary and atoll source GX 9+1 from archival Chandra X-ray Observatory data. The new position significantly differs from a previously published Chandra position for this source. Based on the revised X-ray...
Main Authors: | van den Berg, Maureen (Author), Homan, Jeroen (Contributor) |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2017-06-08T17:43:09Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
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) -
The Disk Wind in the Neutron Star Low-mass X-Ray Binary GX 13+1
by: Allen, Jessamyn Leigh, et al.
Published: (2019) -
THE SPECTRAL EVOLUTION ALONG THE Z TRACK OF THE BRIGHT NEUTRON STAR X-RAY BINARY GX 17+2
by: Lin, Dacheng, et al.
Published: (2015) -
A VARIABLE NEAR-INFRARED COUNTERPART TO THE NEUTRON-STAR LOW-MASS X-RAY BINARY 4U 1705 - 440
by: Homan, Jeroen, et al.
Published: (2015) -
AN ULTRA-FAST X-RAY DISK WIND IN THE NEUTRON STAR BINARY GX 340+0
by: Miller, J. M., et al.
Published: (2017)