Name | 088135 |
Title | Physics and Energetics of the Ultra Fast Outflow in IRAS F11119+3257 |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881350101 |
DOI | https://doi.org/10.57780/esa-g4cshz7 |
Author | Dr Giorgio Lanzuisi |
Description | IRASF11119+3257 is an Ultra Luminous Infrared Galaxy (ULIRG) with post merger morphology, hosting a type-1 QSO (LX 10^44 erg/s at z=0.189) with a persistent UFO (v 0.25c) observed with both NuSTAR and Suzaku. It is also the first system in which it was possible to connect the nuclear outflow with a galaxy-scale molecular outflow, observed in OH and CO transitions. Despite its exceptional properties, the source was never observed with XMM-Newton. We request a 110ks XMM-Newton observation to study in detail the nuclear outflow properties and energetics. We also request 53 ks of simultaneous NuSTAR observation, which is crucial in order to constrain the blue wing of the UFO, and the absorption edges and continuum above 10 keV. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2021-11-12T07:15:26Z/2021-11-13T17:57:17Z |
Version | 19.16_20210326_1200 |
Mission Description | The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 | 2022-12-21T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Giorgio Lanzuisi, 2022, 088135, 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-g4cshz7 |