2020
DOI: 10.17576/jkukm-2020-si3(1)-02
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X-ray Sources Population in NGC 1559

Abstract: We present Chandra observation of the nearby spiral galaxy NGC 1559 to study the X-ray sources population in the galaxy. Based on our analysis, we detect twenty-four X-ray sources in the galaxy, of which six have 0.5–8 keV luminosities exceeding 10<sup>39</sup> erg s<sup>-1</sup>, suggesting that they are possibly ultra-luminous X-ray source (ULX) candidates. The remaining eighteen sources have 0.5–8 keV luminosities below this threshold value, suggesting that they are likely to be X-ra… Show more

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