A mysterious feature in the NICER spectrum of 4U 1820-30: A gravitationally redshifted absorption line?
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| Main Authors: | , , , , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866915637538848768 |
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| author | Iaria, R. Di Salvo, T. Anitra, A. Barra, F. Sanna, A. Maraventano, C. Miceli, C. Leone, W. Burderi, L. |
| author_facet | Iaria, R. Di Salvo, T. Anitra, A. Barra, F. Sanna, A. Maraventano, C. Miceli, C. Leone, W. Burderi, L. |
| contents | A mysterious absorption feature at approximately 3.8 keV has been identified in the NICER spectrum of the low-mass X-ray binary system 4U 1820-30. We interpret this feature as a gravitationally redshifted iron absorption line. This interpretation is supported by the temporal proximity of the NICER observation to the detection of a carbon superburst by the X-ray monitor MAXI, suggesting that the presence of the line is associated with this rare and extreme event. From the inferred redshift of the absorption line, the compactness of the neutron star can be derived. Using a photoionization absorption model, we measure a gravitational redshift of about 1.72, which corresponds to a compactness R/M of 4.46 \pm 0.13 km per solar mass, or 3.02 \pm 0.09 in dimensionless units. This unique feature highlights the importance of further observations and detailed modelling, offering promising insights into the equation of state of matter under extreme density conditions. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2511_20499 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | A mysterious feature in the NICER spectrum of 4U 1820-30: A gravitationally redshifted absorption line? Iaria, R. Di Salvo, T. Anitra, A. Barra, F. Sanna, A. Maraventano, C. Miceli, C. Leone, W. Burderi, L. High Energy Astrophysical Phenomena A mysterious absorption feature at approximately 3.8 keV has been identified in the NICER spectrum of the low-mass X-ray binary system 4U 1820-30. We interpret this feature as a gravitationally redshifted iron absorption line. This interpretation is supported by the temporal proximity of the NICER observation to the detection of a carbon superburst by the X-ray monitor MAXI, suggesting that the presence of the line is associated with this rare and extreme event. From the inferred redshift of the absorption line, the compactness of the neutron star can be derived. Using a photoionization absorption model, we measure a gravitational redshift of about 1.72, which corresponds to a compactness R/M of 4.46 \pm 0.13 km per solar mass, or 3.02 \pm 0.09 in dimensionless units. This unique feature highlights the importance of further observations and detailed modelling, offering promising insights into the equation of state of matter under extreme density conditions. |
| title | A mysterious feature in the NICER spectrum of 4U 1820-30: A gravitationally redshifted absorption line? |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2511.20499 |