A dataset provided by the European Space Agency

Proposal ID 093085
Title PROBING ACCRETION DISK STRUCTURE IN THE INTERMEDIATE-MASS X-RAY BINARY 4U 1210-6
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0930850101

DOI https://doi.org/10.57780/esa-ix6t4wt
Principal Investigator, PI Dr Joel Coley
Abstract We propose contemporaneous NuSTAR and XMM-Newton observations of the recentlyclassified IMXB 4U 1210-64 for 40 ks. Taking advantage of the excellent timingand spectral resolution of NuSTAR, we will perform broadband continuumspectroscopy and look for signatures of a NS or BH such as pulsations, QPOs andCRSFs. With XMM-Newton, we will probe the geometry and ionization structure ofthe accretion flow onto the compact object using the high spectral resolution ofRGS; measure the profile of the Fe Kalpha, Fe XXV and Fe XXVI emission lines aswell as search for emission lines of lower Z ions. Our observation of 4U 1210-64holds broader astrophysical r^ance in characterizing the circumstellarenvironment in IMXBs and will be the first observation of 4U1210 with grating resolution.
Publications No publications found for current proposal!
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2023-12-30T05:51:24Z/2023-12-30T18:21:04Z
Version 21.23_20231215_1101
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2025-01-16T00:00:00Z
Last Update 2025-01-27
Keywords XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Joel Coley, 2025, 'PROBING ACCRETION DISK STRUCTURE IN THE INTERMEDIATE-MASS X-RAY BINARY 4U 1210-6', 21.23_20231215_1101, European Space Agency, https://doi.org/10.57780/esa-ix6t4wt