| Proposal ID | 088486 |
| Title | Using the newly discovered X-ra- IR Type-I bursts to probe jet-disk interaction |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0884860101 |
| DOI | https://doi.org/10.57780/esa-atimc5y |
| Principal Investigator, PI | Dr Federico Vincentelli |
| Abstract | During AO 18 our team discovered the presence of two IR bursts laggingthermonuclear Type-I X-ray bursts\: this allowed us to put the first constraintson the orbital period of the source 4U 1728-34. Moreover, the profiles of thenewly discovered IR bursts showed intriguing .dips. just after the onset of theX-ray bursts. The aim of this proposal is to use the novel method of X-ray-IRburst lag to measure the orbital period of 4U 1728-34 and two other sources, andto quantify the presence of .dips. in their IR reverberation, signatures thatwould indicate burst-induced changes in the geometry of the accretion flow. Wetherefore ask to perform 4 (total 56ks) XMM pointings to be matched by 4 (total14h) HAWK-I@VLT observations of 4U 1728-34, 4U 1705-44 and 4U 1636-53. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2021-09-10T00:00:53Z/2021-09-10T08:12:39Z |
| Version | 19.17_20220121_1250 |
| 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 | 2022-10-02T00:00:00Z |
| Keywords | "novel method", "burst induced", "total 14h hawk", "XMM", "xray bursts", "xmm pointings", "ir reverberation", "4u 1705", "source 4u 1728", "accretion flow", "4u 1636", "xray bursts \:", "orbital period", "4u 1728", "ir bursts" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Federico Vincentelli, 2022, 'Using the newly discovered X-ra- IR Type-I bursts to probe jet-disk interaction', 19.17_20220121_1250, European Space Agency, https://doi.org/10.57780/esa-atimc5y |