Abstract
AX J1745.6-2901 and GRS 1741-2853 are two transient neutron star low-mass X-ray binaries that are located within ≃ 10′ from the Galactic center. Multi-year monitoring observations with the Swift/XRT has exposed several accretion outbursts from these objects. We report on their updated X-ray light curves and renewed activity that occurred in 2010-2013.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 315-317 |
| Number of pages | 3 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 9 |
| Issue number | S303 |
| DOIs | |
| State | Published - May 2014 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
-
SDG 3 Good Health and Well-being
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Fingerprint
Dive into the research topics of 'The Galactic center X-ray transients AX J1745.6-2901 and GRS 1741-2853'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver