Abstract
We present Neutron Star Interior Composition Explorer (NICER) observations of the neutron star (NS) low-mass X-ray binary Serpens X-1 during the early mission phase in 2017. With the high spectral sensitivity and low-energy X-ray passband of NICER, we are able to detect the Fe L line complex in addition to the signature broad, asymmetric Fe K line. We confirm the presence of these lines by comparing the NICER data to archival observations with XMM-Newton/Reflection Grating Spectrometer (RGS) and NuSTAR.
Original language | English |
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Article number | L5 |
Journal | Astrophysical Journal Letters |
Volume | 858 |
Issue number | 1 |
Number of pages | 6 |
ISSN | 2041-8205 |
DOIs | |
Publication status | Published - 2018 |
Keywords
- Accretion
- Accretion disks
- Stars: individual (Ser X-1)
- Stars: neutron
- X-rays: binaries