XMM-Newton and NuSTAR discovery of a likely IP candidate XMMU J173029.8–330920 in the Galactic disc

[Aims] We aim to characterise the population of low-luminosity X-ray sources in the Galactic plane by studying their X-ray spectra and periodic signals in the light curves.

Bibliographic Details
Authors: Mondal, Samaresh, Ponti, Gabriele, Filor, Luke, Bao, Tong, Haberl, Frank, Salcedo, Ciro, Campana, Sergio, Hailey, Charles J., Mori, Kaya, Rea, Nanda
Format: article
Status:Published version
Publication Date:2024
Country:España
Institution:Consejo Superior de Investigaciones Científicas (CSIC)
Repository:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/371845
Online Access:http://hdl.handle.net/10261/371845
Access Level:Open access
Keyword:Binaries: close
Novae
Cataclysmic variables
White dwarfs
Galaxy: center
Galaxy: disk
Description
Summary:[Aims] We aim to characterise the population of low-luminosity X-ray sources in the Galactic plane by studying their X-ray spectra and periodic signals in the light curves.

Similar Items